This analysis is done by the script util/transients/transient_factory_test31.sh /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 11.96 22:09:24.00 +47:56:36.1
96.95443 -6.58680 galactic Lac Second-epoch detections are separated by 7.2" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1975711108228238848 | 22:09:20.94 +47:56:44.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1975711108228238848,2461061.5558,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1975711108228238848 20260121.0558 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:09:24.00 +47:56:36.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2165012650793960832,2461061.5558,10.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2165012650793960832 20260121.0558 10.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:22:33.84 +48:57:03.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 10.78 22:19:28.00 +50:11:11.7
99.59872 -5.67212 galactic Lac Second-epoch detections are separated by 6.0" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2000091679064936960 | 22:19:24.87 +50:11:26.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2000091679064936960,2461061.5558,10.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2000091679064936960 20260121.0558 10.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:19:28.00 +50:11:11.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 11.37 21:31:22.14 +48:26:44.0
92.35869 -2.18429 galactic Cyg Second-epoch detections are separated by 6.9" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1978647525817035776 | 21:31:20.35 +48:27:11.8 (Gaia DR3) | S (local) | (local) | Gaia3var=NOT_AVAILABLE SpType: A7 1940AN....270..201M NGC 7092 57
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1978647525817035776,2461061.5558,11.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1978647525817035776 20260121.0558 11.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:31:22.14 +48:26:44.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1976857864500173312,2461061.5558,11.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1976857864500173312 20260121.0558 11.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:03:43.48 +49:45:23.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 11.47 22:08:59.96 +48:32:00.5
97.24556 -6.06819 galactic Lac Second-epoch detections are separated by 6.1" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J332.2631+48.5283 | 22:08:59.10 +48:32:02.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J332.2631+48.5283,2461061.5558,11.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J332.2631+48.5283 20260121.0558 11.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:08:59.96 +48:32:00.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1978788606919679104,2461061.5558,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1978788606919679104 20260121.0558 11.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:38:00.57 +48:28:18.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1977602817979125248,2461061.5558,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1977602817979125248 20260121.0558 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:36:35.43 +47:32:50.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J212902.91+511421.0,2461061.5558,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J212902.91+511421.0 20260121.0558 11.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:29:03.93 +51:14:20.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 11.88 21:57:08.84 +49:52:16.7
96.49323 -3.83776 galactic Cyg Second-epoch detections are separated by 7.9" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.2760+49.8595 | 21:57:06.68 +49:51:56.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.2760+49.8595,2461061.5558,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.2760+49.8595 20260121.0558 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:57:08.84 +49:52:16.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
AT Lac,2461061.5558,11.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
AT Lac 20260121.0558 11.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:10:58.49 +46:27:24.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Mis V1035,2461061.5558,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Mis V1035 20260121.0558 12.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:29:40.60 +49:49:53.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 12.10 22:16:36.54 +49:26:23.5
98.79658 -6.03732 galactic Lac Second-epoch detections are separated by 6.1" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1999908404219986560 | 22:16:35.47 +49:26:26.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1999908404219986560,2461061.5558,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1999908404219986560 20260121.0558 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:16:36.54 +49:26:23.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 12.09 21:28:03.62 +49:15:08.4
92.51664 -1.22397 galactic Cyg Second-epoch detections are separated by 8.9" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J322.0096+49.2531 | 21:28:04.16 +49:14:45.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J322.0096+49.2531,2461061.5558,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J322.0096+49.2531 20260121.0558 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:28:03.62 +49:15:08.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 12.07 21:38:02.80 +49:24:22.3
93.81746 -2.21400 galactic Cyg Second-epoch detections are separated by 8.4" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J324.5181+49.4098 | 21:38:01.54 +49:24:25.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J324.5181+49.4098,2461061.5558,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J324.5181+49.4098 20260121.0558 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:38:02.80 +49:24:22.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J213741.27+472655.1,2461061.5558,12.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J213741.27+472655.1 20260121.0558 12.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:37:42.38 +47:26:32.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 12.16 22:04:34.59 +49:35:30.8
97.28273 -4.78613 galactic Lac Second-epoch detections are separated by 5.8" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J331.1534+49.5741 | 22:04:34.70 +49:34:54.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J331.1534+49.5741,2461061.5558,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J331.1534+49.5741 20260121.0558 12.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:04:34.59 +49:35:30.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 12.11 21:16:46.25 +44:55:20.8
88.10082 -2.94456 galactic Cyg Second-epoch detections are separated by 6.1" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J319.1868+44.9231 | 21:16:44.85 +44:55:23.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J319.1868+44.9231,2461061.5558,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J319.1868+44.9231 20260121.0558 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:16:46.25 +44:55:20.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 12.15 21:18:09.66 +48:55:21.5
91.13105 -0.32071 galactic Cyg Second-epoch detections are separated by 7.6" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J319.5358+48.9238 | 21:18:08.60 +48:55:26.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J319.5358+48.9238,2461061.5558,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J319.5358+48.9238 20260121.0558 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:18:09.66 +48:55:21.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 12.19 21:34:36.84 +47:42:37.2
92.25778 -3.09211 galactic Cyg Second-epoch detections are separated by 8.1" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J323.6487+47.7165 | 21:34:35.68 +47:42:39.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J323.6487+47.7165,2461061.5558,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J323.6487+47.7165 20260121.0558 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:34:36.84 +47:42:37.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1978336260968904704,2461061.5558,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1978336260968904704 20260121.0558 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:31:01.06 +47:48:28.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 14.38 21:57:30.89 +48:52:36.7
95.92765 -4.65897 galactic Cyg Second-epoch detections are separated by 5.9" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.3645+48.8755 | 21:57:30.89 +48:52:36.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.227+/-0.249 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.3645+48.8755,2461061.5558,14.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.3645+48.8755 20260121.0558 14.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:57:30.89 +48:52:36.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 14.39 21:33:16.38 +50:28:31.5
93.96613 -0.90596 galactic Cyg Second-epoch detections are separated by 7.7" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J323.3110+50.4820 | 21:33:16.38 +50:28:31.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: A1V (LAMOST DR5) J-Ks=0.591+/-0.095 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J323.3110+50.4820,2461061.5558,14.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J323.3110+50.4820 20260121.0558 14.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:33:16.38 +50:28:31.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.5558,14.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.0558 14.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:05:11.47 +47:42:15.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.5558,14.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.0558 14.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:19:58.30 +45:10:47.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 14.35 22:03:51.19 +49:54:45.9
97.38014 -4.45875 galactic Lac Second-epoch detections are separated by 5.9" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J330.9608+49.9124 | 22:03:51.19 +49:54:45.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J330.9608+49.9124,2461061.5558,14.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J330.9608+49.9124 20260121.0558 14.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:03:51.19 +49:54:45.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 14.24 21:49:17.71 +49:23:01.1
95.19361 -3.42263 galactic Cyg Second-epoch detections are separated by 6.7" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J327.3172+49.3841 | 21:49:17.71 +49:23:01.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J327.3172+49.3841,2461061.5558,14.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J327.3172+49.3841 20260121.0558 14.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:49:17.71 +49:23:01.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1978192809054855296,2461061.5558,14.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1978192809054855296 20260121.0558 14.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:45:56.74 +49:22:20.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.5558,14.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.0558 14.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:19:35.35 +50:03:18.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 14.29 22:19:38.00 +49:22:09.1
99.16873 -6.36925 galactic Lac Second-epoch detections are separated by 8.4" and 9.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J334.9069+49.3763 | 22:19:38.00 +49:22:09.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J334.9069+49.3763,2461061.5558,14.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J334.9069+49.3763 20260121.0558 14.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:19:38.00 +49:22:09.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 14.34 21:53:07.05 +49:51:14.6
95.97211 -3.44842 galactic Cyg Second-epoch detections are separated by 8.6" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J328.2795+49.8583 | 21:53:07.05 +49:51:14.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J328.2795+49.8583,2461061.5558,14.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J328.2795+49.8583 20260121.0558 14.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:53:07.05 +49:51:14.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 14.21 21:44:47.73 +48:08:29.5
93.82453 -3.89787 galactic Cyg Second-epoch detections are separated by 8.3" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J326.1981+48.1330 | 21:44:47.73 +48:08:29.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J326.1981+48.1330,2461061.5558,14.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J326.1981+48.1330 20260121.0558 14.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:44:47.73 +48:08:29.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 14.29 21:18:34.06 +45:49:10.8
88.96436 -2.54380 galactic Cyg Second-epoch detections are separated by 5.5" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J319.6434+45.8251 | 21:18:34.06 +45:49:10.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J319.6434+45.8251,2461061.5558,14.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J319.6434+45.8251 20260121.0558 14.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:18:34.06 +45:49:10.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 14.07 22:09:34.02 +48:54:16.7
97.53917 -5.82071 galactic Lac Second-epoch detections are separated by 7.5" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:09:34.02 +48:54:16.7 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.5558,14.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.0558 14.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:09:34.02 +48:54:16.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.94 22:14:30.31 +50:06:47.7
98.89500 -5.28951 galactic Lac Second-epoch detections are separated by 8.8" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J333.6389+50.0961 | 22:14:29.42 +50:06:08.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J333.6389+50.0961,2461061.5558,13.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J333.6389+50.0961 20260121.0558 13.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:14:30.31 +50:06:47.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1979615955059966336,2461061.5558,13.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1979615955059966336 20260121.0558 13.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:49:48.93 +49:04:58.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.96 22:01:36.12 +48:24:46.3
96.18156 -5.43813 galactic Cyg Second-epoch detections are separated by 5.1" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J330.3945+48.4133 | 22:01:38.71 +48:24:50.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.784+/- (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J330.3945+48.4133,2461061.5558,13.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J330.3945+48.4133 20260121.0558 13.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:01:36.12 +48:24:46.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1978736551924644224,2461061.5558,13.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1978736551924644224 20260121.0558 13.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:33:20.18 +49:05:12.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.82 21:33:45.84 +46:50:32.7
91.56361 -3.63420 galactic Cyg Second-epoch detections are separated by 8.6" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J323.4332+46.8457 | 21:33:48.18 +46:50:34.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J323.4332+46.8457,2461061.5558,13.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J323.4332+46.8457 20260121.0558 13.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:33:45.84 +46:50:32.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.87 21:36:56.22 +47:53:16.9
92.66673 -3.22258 galactic Cyg Second-epoch detections are separated by 7.1" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J324.2250+47.8845 | 21:36:56.22 +47:53:16.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J324.2250+47.8845,2461061.5558,13.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J324.2250+47.8845 20260121.0558 13.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:36:56.22 +47:53:16.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1978112304186058496,2461061.5558,13.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1978112304186058496 20260121.0558 13.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:49:02.96 +48:55:00.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.5558,13.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.0558 13.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:21:42.68 +48:57:36.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.77 21:49:49.54 +49:09:23.6
95.11592 -3.65294 galactic Cyg Second-epoch detections are separated by 8.3" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ZTF J214943.92+490955.4 | 21:49:45.84 +49:09:44.3 (Gaia DR3) | EW (local) | 2458632.97060 (local) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J214943.92+490955.4,2461061.5558,13.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J214943.92+490955.4 20260121.0558 13.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:49:49.54 +49:09:23.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1976779352499671936,2461061.5558,13.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1976779352499671936 20260121.0558 13.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:11:29.98 +50:09:32.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.73 21:20:07.52 +50:40:36.9
92.60193 0.68652 galactic Cyg Second-epoch detections are separated by 8.4" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J320.0512+50.6639 | 21:20:09.87 +50:40:14.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J320.0512+50.6639,2461061.5558,13.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J320.0512+50.6639 20260121.0558 13.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:20:07.52 +50:40:36.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.59 21:35:37.63 +48:44:29.8
93.07784 -2.44321 galactic Cyg Second-epoch detections are separated by 8.8" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J323.8923+48.7453 | 21:35:37.63 +48:44:29.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J323.8923+48.7453,2461061.5558,13.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J323.8923+48.7453 20260121.0558 13.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:35:37.63 +48:44:29.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.62 21:24:56.85 +49:22:05.8
92.23180 -0.78837 galactic Cyg Second-epoch detections are separated by 7.6" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J321.2314+49.3561 | 21:24:56.85 +49:22:05.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.484+/-0.280 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J321.2314+49.3561,2461061.5558,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J321.2314+49.3561 20260121.0558 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:24:56.85 +49:22:05.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.62 21:50:32.05 +49:00:12.0
95.10845 -3.84498 galactic Cyg Second-epoch detections are separated by 7.8" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:50:32.05 +49:00:12.0 (user input) | T | P | (position from user input) J-Ks=0.396+/-0.175 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.5558,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.0558 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:50:32.05 +49:00:12.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1975698807440779648,2461061.5558,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1975698807440779648 20260121.0558 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:06:18.73 +47:53:23.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.5558,13.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.0558 13.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:10:39.36 +49:10:57.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.5558,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.0558 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:05:30.06 +50:16:21.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.34 21:42:30.48 +50:06:53.7
94.82718 -2.15666 galactic Cyg Second-epoch detections are separated by 8.7" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1979039089411627392 | 21:42:28.18 +50:06:38.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1979039089411627392,2461061.5558,13.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1979039089411627392 20260121.0558 13.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:42:30.48 +50:06:53.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.20 21:59:40.89 +49:13:35.1
96.42390 -4.59937 galactic Cyg Second-epoch detections are separated by 7.0" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.9134+49.2261 | 21:59:40.89 +49:13:35.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.557+/-0.200 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.9134+49.2261,2461061.5558,13.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.9134+49.2261 20260121.0558 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:59:40.89 +49:13:35.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.29 22:13:09.21 +48:36:54.3
97.85767 -6.39769 galactic Lac Second-epoch detections are separated by 7.0" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 | 22:13:08.41 +48:36:35.7 (Gaia DR3) | 1975849234377049216 (VSX @ VizieR) | S (VSX @ VizieR) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3,2461061.5558,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 20260121.0558 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:13:09.21 +48:36:54.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.03 21:05:44.65 +46:40:00.2
88.05953 -0.34967 galactic Cyg Second-epoch detections are separated by 8.5" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J316.4312+46.6663 | 21:05:44.65 +46:40:00.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J316.4312+46.6663,2461061.5558,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J316.4312+46.6663 20260121.0558 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:05:44.65 +46:40:00.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.5558,13.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.0558 13.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:01:31.94 +48:35:21.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.5558,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.0558 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:08:56.39 +45:19:51.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J222119.36+495736.0,2461061.5558,13.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J222119.36+495736.0 20260121.0558 13.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:21:19.82 +49:57:43.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 12.84 21:33:52.27 +49:00:09.4
93.04039 -2.05579 galactic Cyg Second-epoch detections are separated by 6.3" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J323.4607+49.0019 | 21:33:52.27 +49:00:09.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J323.4607+49.0019,2461061.5558,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J323.4607+49.0019 20260121.0558 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:33:52.27 +49:00:09.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.14 21:57:50.94 +48:39:54.0
95.84071 -4.85999 galactic Cyg Second-epoch detections are separated by 0.3" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1976402524936085632 | 21:57:49.25 +48:40:12.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1976402524936085632,2461061.5558,13.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1976402524936085632 20260121.0558 13.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:57:50.94 +48:39:54.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 12.93 21:33:57.57 +50:09:22.1
93.83086 -1.21524 galactic Cyg Second-epoch detections are separated by 5.3" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J323.4982+50.1519 | 21:33:56.59 +50:09:24.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J323.4982+50.1519,2461061.5558,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J323.4982+50.1519 20260121.0558 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:33:57.57 +50:09:22.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.5558,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.0558 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:05:55.03 +45:20:51.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 12.86 21:38:53.58 +48:47:51.2
93.51623 -2.76086 galactic Cyg Second-epoch detections are separated by 7.7" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J324.7202+48.7946 | 21:38:53.58 +48:47:51.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J324.7202+48.7946,2461061.5558,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J324.7202+48.7946 20260121.0558 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:38:53.58 +48:47:51.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 12.86 22:04:52.15 +50:07:30.4
97.63840 -4.38506 galactic Lac Second-epoch detections are separated by 4.1" and 9.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J331.2155+50.1442 | 22:04:51.18 +50:07:54.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J331.2155+50.1442,2461061.5558,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J331.2155+50.1442 20260121.0558 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:04:52.15 +50:07:30.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 12.72 21:32:27.17 +50:37:43.1
93.97433 -0.70501 galactic Cyg Second-epoch detections are separated by 6.0" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2171396793265581952 | 21:32:25.17 +50:38:05.3 (Gaia DR3) | DSCT/GDOR (local) | (local) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2171396793265581952,2461061.5558,12.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2171396793265581952 20260121.0558 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:32:27.17 +50:37:43.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 12.43 21:50:22.53 +49:03:02.2
95.11829 -3.79192 galactic Cyg Second-epoch detections are separated by 5.6" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J327.5837+49.0501 | 21:50:19.67 +49:02:55.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J327.5837+49.0501,2461061.5558,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J327.5837+49.0501 20260121.0558 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:50:22.53 +49:03:02.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1979995316625158144,2461061.5558,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1979995316625158144 20260121.0558 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:59:47.18 +50:39:15.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1999965029071193728,2461061.5558,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1999965029071193728 20260121.0558 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:15:28.90 +49:43:47.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 11.30 21:44:58.05 +46:33:37.0
92.81719 -5.11966 galactic Cyg Second-epoch detections are separated by 5.8" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J326.2548+46.5476 | 21:44:58.34 +46:33:05.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J326.2548+46.5476,2461061.5558,11.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J326.2548+46.5476 20260121.0558 11.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:44:58.05 +46:33:37.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 11.54 22:16:03.39 +45:04:29.0
96.23860 -9.59304 galactic Lac Second-epoch detections are separated by 7.3" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1962222093414152448 | 22:16:02.62 +45:04:31.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1962222093414152448,2461061.5558,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1962222093414152448 20260121.0558 11.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:16:03.39 +45:04:29.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 11.46 21:52:51.40 +49:52:30.6
95.95252 -3.40564 galactic Cyg Second-epoch detections are separated by 6.9" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J328.2029+49.8566 | 21:52:49.42 +49:52:05.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G0 1952CoRut..32....1H BD+49 3653
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J328.2029+49.8566,2461061.5558,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J328.2029+49.8566 20260121.0558 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:52:51.40 +49:52:30.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 11.65 21:24:52.88 +46:30:02.7
90.22075 -2.83361 galactic Cyg Second-epoch detections are separated by 6.8" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 varaible 1972153157320885248 | 21:24:51.69 +46:29:19.0 (Gaia DR3) | DSCT/GDOR/SXPHE (Gaia DR3) | 2022yCat.1358....0G | Gaia3var=VARIABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') SpType: F0 1960UppAn...4h...1M BD+45 3529
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 varaible 1972153157320885248,2461061.5558,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 varaible 1972153157320885248 20260121.0558 11.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:24:52.88 +46:30:02.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 11.78 22:15:12.47 +49:53:15.4
98.86072 -5.53951 galactic Lac Second-epoch detections are separated by 2.0" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1999981453026026880 | 22:15:10.80 +49:52:40.3 (Gaia DR3) | DSCT/GDOR (local) | B (local) | Gaia3var=VARIABLE SpType: B8? 1940AN....270..201M Cl* NGC 7243 M 55
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1999981453026026880,2461061.5558,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1999981453026026880 20260121.0558 11.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:15:12.47 +49:53:15.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 11.85 21:56:48.27 +47:22:53.7
94.90901 -5.76389 galactic Cyg Second-epoch detections are separated by 5.0" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.1981+47.3817 | 21:56:50.03 +47:23:06.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.1981+47.3817,2461061.5558,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.1981+47.3817 20260121.0558 11.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:56:48.27 +47:22:53.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1976050685521737216,2461061.5558,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1976050685521737216 20260121.0558 11.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:54:42.38 +47:29:35.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1976205338708921600,2461061.5558,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1976205338708921600 20260121.0558 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:00:48.84 +48:16:17.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 11.93 21:25:18.69 +51:08:01.4
93.50453 0.43654 galactic Cyg Second-epoch detections are separated by 5.4" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | HD 204194 | 21:25:23.10 +51:07:57.3 (Gaia DR3) | VAR (local) | 2457324.52860 (local) | Gaia3var=VARIABLE SpType: A2 1939UppAn...1a...1V BD+50 3333
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HD 204194,2461061.5558,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HD 204194 20260121.0558 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:25:18.69 +51:08:01.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 12.07 22:08:35.16 +47:21:26.9
96.49808 -6.98267 galactic Lac Second-epoch detections are separated by 8.7" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J332.1320+47.3471 | 22:08:31.93 +47:21:24.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J332.1320+47.3471,2461061.5558,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J332.1320+47.3471 20260121.0558 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:08:35.16 +47:21:26.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 12.09 22:02:59.92 +49:59:04.4
97.31259 -4.31906 galactic Lac Second-epoch detections are separated by 3.0" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J330.7433+49.9844 | 22:02:58.24 +49:59:36.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J330.7433+49.9844,2461061.5558,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J330.7433+49.9844 20260121.0558 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:02:59.92 +49:59:04.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 12.17 22:08:01.64 +47:33:12.7
96.53661 -6.76844 galactic Lac Second-epoch detections are separated by 5.9" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J331.9991+47.5605 | 22:07:58.31 +47:33:10.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J331.9991+47.5605,2461061.5558,12.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J331.9991+47.5605 20260121.0558 12.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:08:01.64 +47:33:12.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461061.5558,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260121.0558 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:02:28.29 +48:30:56.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 12.22 21:32:07.69 +49:24:34.9
93.10729 -1.56355 galactic Cyg Second-epoch detections are separated by 7.8" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J323.0118+49.4208 | 21:32:04.42 +49:24:52.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J323.0118+49.4208,2461061.5558,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J323.0118+49.4208 20260121.0558 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:32:07.69 +49:24:34.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 12.33 22:00:58.49 +48:21:35.1
96.06599 -5.41751 galactic Cyg Second-epoch detections are separated by 4.0" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J330.2405+48.3718 | 22:00:58.49 +48:21:35.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J330.2405+48.3718,2461061.5558,12.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J330.2405+48.3718 20260121.0558 12.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:00:58.49 +48:21:35.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 12.36 22:16:29.91 +46:55:36.5
97.36047 -8.10731 galactic Lac Second-epoch detections are separated by 3.8" and 8.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ZTF J221631.86+465503.6 | 22:16:29.66 +46:55:11.8 (Gaia DR3) | RS (local) | 2458366.83370 (local) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J221631.86+465503.6,2461061.5558,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J221631.86+465503.6 20260121.0558 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:16:29.91 +46:55:36.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1979666184685752448,2461061.5558,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1979666184685752448 20260121.0558 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:52:46.20 +49:52:01.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 12.42 21:55:07.97 +50:28:35.4
96.61339 -3.16255 galactic Cyg Second-epoch detections are separated by 5.9" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J328.7707+50.4849 | 21:55:07.03 +50:28:36.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J328.7707+50.4849,2461061.5558,12.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J328.7707+50.4849 20260121.0558 12.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:55:07.97 +50:28:35.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 12.39 21:55:13.78 +47:26:01.8
94.73138 -5.55778 galactic Cyg Second-epoch detections are separated by 6.8" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1976052231712686976 | 21:55:12.82 +47:26:03.0 (Gaia DR3) | RS (local) | (local) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1976052231712686976,2461061.5558,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1976052231712686976 20260121.0558 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:55:13.78 +47:26:01.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 12.43 22:03:43.54 +49:44:21.3
97.25979 -4.58576 galactic Lac Second-epoch detections are separated by 6.0" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J330.9244+49.7348 | 22:03:43.54 +49:44:21.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J330.9244+49.7348,2461061.5558,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J330.9244+49.7348 20260121.0558 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:03:43.54 +49:44:21.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J214113.32+473358.3,2461061.5558,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J214113.32+473358.3 20260121.0558 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:41:14.27 +47:33:54.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 12.54 22:15:25.93 +46:12:35.8
96.79857 -8.59558 galactic Lac Second-epoch detections are separated by 4.6" and 8.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J333.8449+46.2124 | 22:15:25.93 +46:12:35.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J333.8449+46.2124,2461061.5558,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J333.8449+46.2124 20260121.0558 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:15:25.93 +46:12:35.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 12.60 22:09:08.10 +50:24:06.2
98.35489 -4.56125 galactic Lac Second-epoch detections are separated by 5.1" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1976994513184406400 | 22:09:07.39 +50:24:48.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1976994513184406400,2461061.5558,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1976994513184406400 20260121.0558 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:09:08.10 +50:24:06.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 12.50 21:37:10.69 +51:04:53.7
94.83075 -0.87226 galactic Cyg Second-epoch detections are separated by 7.5" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J324.2829+51.0824 | 21:37:09.64 +51:04:56.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J324.2829+51.0824,2461061.5558,12.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J324.2829+51.0824 20260121.0558 12.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:37:10.69 +51:04:53.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.5558,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.0558 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:10:27.25 +47:08:57.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2165607074267249280,2461061.5558,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2165607074267249280 20260121.0558 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:05:51.35 +48:46:20.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 12.57 21:55:57.01 +45:55:06.9
93.88159 -6.82171 galactic Cyg Second-epoch detections are separated by 3.5" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1973622860765272960 | 21:55:54.92 +45:54:28.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1973622860765272960,2461061.5558,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1973622860765272960 20260121.0558 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:55:57.01 +45:55:06.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J213134.46+483310.7,2461061.5558,12.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J213134.46+483310.7 20260121.0558 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:31:35.57 +48:33:08.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 12.69 22:05:14.44 +49:19:47.5
97.21384 -5.06107 galactic Lac Second-epoch detections are separated by 7.3" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J331.3085+49.3352 | 22:05:14.44 +49:19:47.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J331.3085+49.3352,2461061.5558,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J331.3085+49.3352 20260121.0558 12.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:05:14.44 +49:19:47.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.5558,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.0558 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:49:11.06 +49:42:07.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1999698328778312576,2461061.5558,12.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1999698328778312576 20260121.0558 12.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:17:30.22 +49:05:44.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 12.76 22:13:32.94 +49:21:46.4
98.33968 -5.82001 galactic Lac Second-epoch detections are separated by 8.5" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J333.4011+49.3662 | 22:13:32.31 +49:22:13.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J333.4011+49.3662,2461061.5558,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J333.4011+49.3662 20260121.0558 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:13:32.94 +49:21:46.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 12.66 21:43:31.56 +47:02:44.9
92.94655 -4.59054 galactic Cyg Second-epoch detections are separated by 6.9" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.8771+47.0463 | 21:43:31.56 +47:02:44.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.8771+47.0463,2461061.5558,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.8771+47.0463 20260121.0558 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:43:31.56 +47:02:44.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 12.77 22:16:03.72 +49:42:40.2
98.87558 -5.76292 galactic Lac Second-epoch detections are separated by 5.7" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1999962658249297024 | 22:16:02.20 +49:43:10.6 (Gaia DR3) | E (local) | A (local) | Gaia3var=NOT_AVAILABLE SpType: F8 1940AN....270..201M Cl* NGC 7243 M 103
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1999962658249297024,2461061.5558,12.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1999962658249297024 20260121.0558 12.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:16:03.72 +49:42:40.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 12.66 21:31:32.27 +45:31:26.7
90.38140 -4.33818 galactic Cyg Second-epoch detections are separated by 1.6" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J322.8968+45.5249 | 21:31:34.42 +45:30:59.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J322.8968+45.5249,2461061.5558,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J322.8968+45.5249 20260121.0558 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:31:32.27 +45:31:26.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.5558,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.0558 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:34:30.99 +50:02:10.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 12.80 22:08:16.30 +47:27:17.2
96.51201 -6.87264 galactic Lac Second-epoch detections are separated by 8.3" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J332.0632+47.4485 | 22:08:12.42 +47:27:09.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J332.0632+47.4485,2461061.5558,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J332.0632+47.4485 20260121.0558 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:08:16.30 +47:27:17.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 12.75 21:33:03.90 +46:29:15.3
91.23413 -3.81361 galactic Cyg Second-epoch detections are separated by 7.2" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J323.2506+46.4852 | 21:33:03.90 +46:29:15.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J323.2506+46.4852,2461061.5558,12.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J323.2506+46.4852 20260121.0558 12.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:33:03.90 +46:29:15.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J215232.51+472307.1,2461061.5558,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J215232.51+472307.1 20260121.0558 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:52:33.39 +47:23:05.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 12.85 22:15:54.10 +49:56:34.4
98.98475 -5.55662 galactic Lac Second-epoch detections are separated by 4.1" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J333.9768+49.9472 | 22:15:51.48 +49:57:14.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G4 1940AN....270..201M Cl* NGC 7243 M 91
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J333.9768+49.9472,2461061.5558,12.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J333.9768+49.9472 20260121.0558 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:15:54.10 +49:56:34.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1977240666341962752,2461061.5558,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1977240666341962752 20260121.0558 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:39:15.74 +46:09:07.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 12.86 22:12:19.43 +46:02:54.3
96.25829 -8.42064 galactic Lac Second-epoch detections are separated by 4.2" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J333.0963+46.0470 | 22:12:20.03 +46:03:06.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J333.0963+46.0470,2461061.5558,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J333.0963+46.0470 20260121.0558 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:12:19.43 +46:02:54.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 12.81 21:57:48.10 +48:21:14.5
95.64288 -5.10067 galactic Cyg Second-epoch detections are separated by 5.4" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.4462+48.3543 | 21:57:48.49 +48:21:40.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.4462+48.3543,2461061.5558,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.4462+48.3543 20260121.0558 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:57:48.10 +48:21:14.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 12.88 22:04:05.93 +47:17:57.4
95.84589 -6.58008 galactic Lac Second-epoch detections are separated by 7.1" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J331.0239+47.3171 | 22:04:07.06 +47:18:39.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J331.0239+47.3171,2461061.5558,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J331.0239+47.3171 20260121.0558 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:04:05.93 +47:17:57.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1979282734316976896,2461061.5558,12.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1979282734316976896 20260121.0558 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:38:39.35 +50:28:43.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1977729364892785664,2461061.5558,12.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1977729364892785664 20260121.0558 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:43:30.07 +47:25:06.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 12.89 21:37:47.60 +50:21:02.9
94.41612 -1.48192 galactic Cyg Second-epoch detections are separated by 7.9" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J324.4406+50.3565 | 21:37:49.60 +50:21:18.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J324.4406+50.3565,2461061.5558,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J324.4406+50.3565 20260121.0558 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:37:47.60 +50:21:02.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 12.92 21:48:56.54 +48:46:40.7
94.76243 -3.85275 galactic Cyg Second-epoch detections are separated by 8.6" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ASASSN-V J214900.08+484711.9 | 21:49:00.08 +48:47:12.0 (Gaia DR3) | SR (local) | 435.000000000000 (local) | Gaia3var=VARIABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J214900.08+484711.9,2461061.5558,12.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J214900.08+484711.9 20260121.0558 12.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:48:56.54 +48:46:40.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 12.99 22:17:05.71 +48:14:32.1
98.18887 -7.07471 galactic Lac Second-epoch detections are separated by 7.1" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1999599647607480448 | 22:17:02.85 +48:14:13.8 (Gaia DR3) | DSCT/GDOR (local) | A (local) | Gaia3var=VARIABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1999599647607480448,2461061.5558,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1999599647607480448 20260121.0558 12.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:17:05.71 +48:14:32.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J221147.70+501139.3,2461061.5558,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J221147.70+501139.3 20260121.0558 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:11:48.82 +50:11:36.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 12.96 22:16:53.79 +46:25:17.3
97.13039 -8.56360 galactic Lac Second-epoch detections are separated by 8.8" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1963180042924983552 | 22:16:52.04 +46:25:51.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1963180042924983552,2461061.5558,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1963180042924983552 20260121.0558 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:16:53.79 +46:25:17.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1978554617106933120,2461061.5558,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1978554617106933120 20260121.0558 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:30:25.14 +48:22:02.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J221856.37+500948.2,2461061.5558,13.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J221856.37+500948.2 20260121.0558 13.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:18:55.53 +50:09:36.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 12.99 22:03:00.32 +47:33:04.6
95.84874 -6.26750 galactic Lac Second-epoch detections are separated by 7.0" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J330.7357+47.5480 | 22:03:00.32 +47:33:04.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J330.7357+47.5480,2461061.5558,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J330.7357+47.5480 20260121.0558 12.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:03:00.32 +47:33:04.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.5558,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.0558 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:46:36.03 +45:43:28.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1963424443744038784,2461061.5558,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1963424443744038784 20260121.0558 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:11:55.77 +47:06:03.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 12.97 21:38:36.85 +47:44:23.4
92.77793 -3.52078 galactic Cyg Second-epoch detections are separated by 6.6" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J324.6524+47.7405 | 21:38:36.85 +47:44:23.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J324.6524+47.7405,2461061.5558,12.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J324.6524+47.7405 20260121.0558 12.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:38:36.85 +47:44:23.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.12 21:33:44.68 +49:37:17.9
93.44397 -1.58577 galactic Cyg Second-epoch detections are separated by 8.7" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J323.4403+49.6188 | 21:33:45.28 +49:36:56.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J323.4403+49.6188,2461061.5558,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J323.4403+49.6188 20260121.0558 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:33:44.68 +49:37:17.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1979280432204369664,2461061.5558,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1979280432204369664 20260121.0558 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:37:53.24 +50:21:38.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.09 22:04:10.07 +50:12:12.5
97.59448 -4.25530 galactic Lac Second-epoch detections are separated by 5.2" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J331.0462+50.2029 | 22:04:09.39 +50:12:46.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J331.0462+50.2029,2461061.5558,13.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J331.0462+50.2029 20260121.0558 13.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:04:10.07 +50:12:12.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.01 22:08:39.80 +48:05:46.3
96.94336 -6.39081 galactic Lac Second-epoch detections are separated by 8.5" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 1975728253737551744 | 22:08:39.87 +48:06:13.9 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 1975728253737551744,2461061.5558,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1975728253737551744 20260121.0558 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:08:39.80 +48:05:46.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163583010811215616,2461061.5558,12.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163583010811215616 20260121.0558 12.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:03.21 +46:16:21.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.07 22:02:22.78 +48:13:16.2
96.16919 -5.66902 galactic Cyg Second-epoch detections are separated by 5.4" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J330.5897+48.2216 | 22:02:25.03 +48:13:10.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J330.5897+48.2216,2461061.5558,13.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J330.5897+48.2216 20260121.0558 13.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:02:22.78 +48:13:16.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.09 20:55:10.62 +48:05:13.3
87.95085 1.93173 galactic Cyg Second-epoch detections are separated by 8.5" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2167013830680893056 | 20:55:12.24 +48:05:03.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2167013830680893056,2461061.5558,13.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2167013830680893056 20260121.0558 13.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:55:10.62 +48:05:13.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1973402168166467200,2461061.5558,13.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1973402168166467200 20260121.0558 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:58:26.39 +45:29:54.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1980634648271731840,2461061.5558,13.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1980634648271731840 20260121.0558 13.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:53:37.35 +50:57:56.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.12 22:14:44.61 +47:06:24.3
97.21390 -7.78984 galactic Lac Second-epoch detections are separated by 4.8" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J333.6735+47.1067 | 22:14:44.61 +47:06:24.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J333.6735+47.1067,2461061.5558,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J333.6735+47.1067 20260121.0558 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:14:44.61 +47:06:24.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.09 21:51:05.66 +49:21:21.6
95.40301 -3.62968 galactic Cyg Second-epoch detections are separated by 7.2" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J327.7524+49.3676 | 21:51:02.78 +49:21:48.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J327.7524+49.3676,2461061.5558,13.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J327.7524+49.3676 20260121.0558 13.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:51:05.66 +49:21:21.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.12 22:00:29.48 +50:31:09.9
97.31441 -3.65069 galactic Cyg Second-epoch detections are separated by 7.3" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1979977969266202752 | 22:00:30.77 +50:30:56.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1979977969266202752,2461061.5558,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1979977969266202752 20260121.0558 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:00:29.48 +50:31:09.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.19 21:56:59.84 +45:47:48.1
93.94960 -7.03037 galactic Cyg Second-epoch detections are separated by 5.6" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.2367+45.7921 | 21:56:59.84 +45:47:48.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.2367+45.7921,2461061.5558,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.2367+45.7921 20260121.0558 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:56:59.84 +45:47:48.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.14 21:38:36.51 +46:16:22.8
91.79896 -4.61535 galactic Cyg Second-epoch detections are separated by 6.1" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J324.6469+46.2668 | 21:38:35.26 +46:16:00.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J324.6469+46.2668,2461061.5558,13.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J324.6469+46.2668 20260121.0558 13.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:38:36.51 +46:16:22.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2171042544360521088,2461061.5558,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2171042544360521088 20260121.0558 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:22:28.52 +49:27:41.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.28 21:59:25.21 +48:33:03.6
95.97700 -5.10902 galactic Cyg Second-epoch detections are separated by 3.1" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.8512+48.5516 | 21:59:25.21 +48:33:03.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.600+/-0.185 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.8512+48.5516,2461061.5558,13.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.8512+48.5516 20260121.0558 13.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:59:25.21 +48:33:03.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.22 21:05:39.74 +47:06:13.7
88.37428 -0.04608 galactic Cyg Second-epoch detections are separated by 8.5" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J316.4245+47.1030 | 21:05:42.24 +47:05:51.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J316.4245+47.1030,2461061.5558,13.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J316.4245+47.1030 20260121.0558 13.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:05:39.74 +47:06:13.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.18 21:35:12.41 +50:06:25.7
93.94553 -1.38617 galactic Cyg Second-epoch detections are separated by 8.6" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2171310000564460288 | 21:35:08.55 +50:06:38.8 (Gaia DR3) | DSCT/GDOR (local) | (local) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2171310000564460288,2461061.5558,13.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2171310000564460288 20260121.0558 13.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:35:12.41 +50:06:25.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1979667185431013376,2461061.5558,13.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1979667185431013376 20260121.0558 13.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:50:46.20 +49:36:28.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.39 22:09:29.63 +50:23:23.1
98.39465 -4.60418 galactic Lac Second-epoch detections are separated by 6.5" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J332.3902+50.3923 | 22:09:31.38 +50:23:34.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J332.3902+50.3923,2461061.5558,13.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J332.3902+50.3923 20260121.0558 13.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:09:29.63 +50:23:23.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.30 21:59:27.84 +48:33:04.8
95.98297 -5.11317 galactic Cyg Second-epoch detections are separated by 3.4" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.8622+48.5522 | 21:59:27.84 +48:33:04.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.8622+48.5522,2461061.5558,13.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.8622+48.5522 20260121.0558 13.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:59:27.84 +48:33:04.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.28 21:36:27.66 +50:01:04.5
94.03496 -1.58737 galactic Cyg Second-epoch detections are separated by 7.2" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J324.1036+50.0115 | 21:36:27.59 +50:00:39.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J324.1036+50.0115,2461061.5558,13.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J324.1036+50.0115 20260121.0558 13.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:36:27.66 +50:01:04.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J221529.54+460819.4,2461061.5558,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J221529.54+460819.4 20260121.0558 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:15:30.75 +46:08:20.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.30 22:15:22.40 +49:29:48.5
98.66170 -5.87749 galactic Lac Second-epoch detections are separated by 8.2" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J333.8319+49.4983 | 22:15:22.40 +49:29:48.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J333.8319+49.4983,2461061.5558,13.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J333.8319+49.4983 20260121.0558 13.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:15:22.40 +49:29:48.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2171042544360521088,2461061.5558,13.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2171042544360521088 20260121.0558 13.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:22:25.99 +49:27:57.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.31 21:51:10.95 +47:10:14.4
94.02879 -5.33235 galactic Cyg Second-epoch detections are separated by 8.6" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J327.8071+47.1723 | 21:51:10.95 +47:10:14.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J327.8071+47.1723,2461061.5558,13.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J327.8071+47.1723 20260121.0558 13.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:51:10.95 +47:10:14.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.32 21:57:49.74 +47:47:55.1
95.30390 -5.54175 galactic Cyg Second-epoch detections are separated by 7.3" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.4518+47.7989 | 21:57:49.74 +47:47:55.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.4518+47.7989,2461061.5558,13.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.4518+47.7989 20260121.0558 13.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:57:49.74 +47:47:55.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1977167200917608832,2461061.5558,13.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1977167200917608832 20260121.0558 13.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:35:39.37 +45:52:31.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J215459.53+481256.9,2461061.5558,13.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J215459.53+481256.9 20260121.0558 13.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:55:01.88 +48:12:57.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.49 21:50:44.50 +48:54:05.0
95.07020 -3.94547 galactic Cyg Second-epoch detections are separated by 7.9" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J327.6721+48.9059 | 21:50:40.54 +48:53:48.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J327.6721+48.9059,2461061.5558,13.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J327.6721+48.9059 20260121.0558 13.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:50:44.50 +48:54:05.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.5558,13.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.0558 13.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:50:21.28 +48:05:24.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.5558,13.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.0558 13.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:38:47.57 +50:34:21.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.32 21:34:43.84 +49:58:23.0
93.79869 -1.43388 galactic Cyg Second-epoch detections are separated by 7.5" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1979153747866863872 | 21:34:43.31 +49:58:01.0 (Gaia DR3) | ROT (local) | (local) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1979153747866863872,2461061.5558,13.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1979153747866863872 20260121.0558 13.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:34:43.84 +49:58:23.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.36 21:27:18.62 +47:03:55.0
90.91301 -2.71741 galactic Cyg Second-epoch detections are separated by 5.2" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J321.8202+47.0606 | 21:27:14.30 +47:04:06.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.170+/- (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J321.8202+47.0606,2461061.5558,13.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J321.8202+47.0606 20260121.0558 13.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:27:18.62 +47:03:55.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2171458636486062464,2461061.5558,13.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2171458636486062464 20260121.0558 13.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:37:19.32 +50:48:11.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.38 21:31:20.36 +45:37:41.5
90.42735 -4.23845 galactic Cyg Second-epoch detections are separated by 4.5" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J322.8302+45.6338 | 21:31:20.36 +45:37:41.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J322.8302+45.6338,2461061.5558,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J322.8302+45.6338 20260121.0558 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:31:20.36 +45:37:41.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.41 22:06:51.07 +47:15:45.3
96.20219 -6.88674 galactic Lac Second-epoch detections are separated by 8.9" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J331.7081+47.2634 | 22:06:51.07 +47:15:45.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J331.7081+47.2634,2461061.5558,13.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J331.7081+47.2634 20260121.0558 13.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:06:51.07 +47:15:45.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.33 20:59:55.91 +45:57:24.0
86.86214 -0.07076 galactic Cyg Second-epoch detections are separated by 4.7" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.9819+45.9568 | 20:59:55.91 +45:57:24.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J314.9819+45.9568,2461061.5558,13.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J314.9819+45.9568 20260121.0558 13.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:59:55.91 +45:57:24.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.38 21:45:56.41 +49:03:16.3
94.56104 -3.32421 galactic Cyg Second-epoch detections are separated by 8.2" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1978172914765850368 | 21:45:55.49 +49:03:49.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1978172914765850368,2461061.5558,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1978172914765850368 20260121.0558 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:45:56.41 +49:03:16.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.5558,13.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.0558 13.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:31:34.94 +45:29:45.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J214101.38+460504.2,2461061.5558,13.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J214101.38+460504.2 20260121.0558 13.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:41:01.04 +46:04:56.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.32 21:35:02.65 +49:00:49.8
93.19006 -2.17727 galactic Cyg Second-epoch detections are separated by 7.9" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J323.7567+49.0109 | 21:34:58.96 +49:01:10.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J323.7567+49.0109,2461061.5558,13.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J323.7567+49.0109 20260121.0558 13.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:35:02.65 +49:00:49.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.45 22:12:32.81 +49:44:00.1
98.41767 -5.42295 galactic Lac Second-epoch detections are separated by 8.5" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1976708640159468160 | 22:12:35.39 +49:43:32.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1976708640159468160,2461061.5558,13.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1976708640159468160 20260121.0558 13.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:12:32.81 +49:44:00.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.35 21:39:18.53 +46:12:13.6
91.84354 -4.74757 galactic Cyg Second-epoch detections are separated by 6.8" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1977245167467671040 | 21:39:15.97 +46:11:52.0 (Gaia DR3) | E (local) | F (local) | Gaia3var=NOT_AVAILABLE J-Ks=0.777+/-0.159 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1977245167467671040,2461061.5558,13.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1977245167467671040 20260121.0558 13.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:39:18.53 +46:12:13.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.37 21:36:33.62 +50:41:05.0
94.49304 -1.10244 galactic Cyg Second-epoch detections are separated by 8.5" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2171362742764068224 | 21:36:31.13 +50:41:29.5 (Gaia DR3) | E (local) | B (local) | Gaia3var=VARIABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2171362742764068224,2461061.5558,13.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2171362742764068224 20260121.0558 13.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:36:33.62 +50:41:05.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.5558,13.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.0558 13.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:22:30.52 +49:27:58.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.45 22:19:14.22 +49:16:18.9
99.06054 -6.41479 galactic Lac Second-epoch detections are separated by 7.9" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1999712244474234624 | 22:19:15.59 +49:16:09.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1999712244474234624,2461061.5558,13.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1999712244474234624 20260121.0558 13.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:19:14.22 +49:16:18.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.44 21:34:28.47 +45:32:04.4
90.76684 -4.68020 galactic Cyg Second-epoch detections are separated by 2.7" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J323.6131+45.5353 | 21:34:28.47 +45:32:04.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J323.6131+45.5353,2461061.5558,13.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J323.6131+45.5353 20260121.0558 13.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:34:28.47 +45:32:04.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.54 22:03:34.59 +49:45:19.6
97.25009 -4.55838 galactic Lac Second-epoch detections are separated by 5.6" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1976904868625540096 | 22:03:36.05 +49:45:57.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1976904868625540096,2461061.5558,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1976904868625540096 20260121.0558 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:03:34.59 +49:45:19.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.53 21:58:48.68 +45:45:43.0
94.17910 -7.25260 galactic Cyg Second-epoch detections are separated by 6.4" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1974919769089688960 | 21:58:51.84 +45:45:52.6 (Gaia DR3) | VAR (local) | M (local) | Gaia3var=VARIABLE SpType: M3 1947AnDea...5....1L DO 40490
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1974919769089688960,2461061.5558,13.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1974919769089688960 20260121.0558 13.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:58:48.68 +45:45:43.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.54 22:15:48.50 +49:55:09.0
98.95888 -5.56781 galactic Lac Second-epoch detections are separated by 8.0" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J333.9478+49.9014 | 22:15:50.13 +49:54:28.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G2 1940AN....270..201M Cl* NGC 7243 M 90
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J333.9478+49.9014,2461061.5558,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J333.9478+49.9014 20260121.0558 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:15:48.50 +49:55:09.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.50 22:05:42.74 +46:42:10.7
95.71074 -7.22292 galactic Lac Second-epoch detections are separated by 7.5" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1975076964896728320 | 22:05:46.14 +46:41:54.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 1940AN....270..201M NGC 7209 108
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1975076964896728320,2461061.5558,13.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1975076964896728320 20260121.0558 13.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:05:42.74 +46:42:10.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.48 21:51:08.21 +46:39:54.0
93.70113 -5.71886 galactic Cyg Second-epoch detections are separated by 7.5" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J327.7812+46.6685 | 21:51:08.61 +46:39:30.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J327.7812+46.6685,2461061.5558,13.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J327.7812+46.6685 20260121.0558 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:51:08.21 +46:39:54.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.54 22:21:22.45 +50:04:20.0
99.79284 -5.93524 galactic Lac Second-epoch detections are separated by 5.8" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J335.3380+50.0619 | 22:21:20.90 +50:03:55.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J335.3380+50.0619,2461061.5558,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J335.3380+50.0619 20260121.0558 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:21:22.45 +50:04:20.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.49 21:58:52.02 +45:46:36.6
94.19604 -7.24680 galactic Cyg Second-epoch detections are separated by 7.7" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1974919769089688960 | 21:58:51.84 +45:45:52.6 (Gaia DR3) | VAR (local) | M (local) | Gaia3var=VARIABLE SpType: M3 1947AnDea...5....1L DO 40490
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1974919769089688960,2461061.5558,13.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1974919769089688960 20260121.0558 13.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:58:52.02 +45:46:36.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.5558,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.0558 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:41:26.39 +50:40:49.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.46 21:42:11.28 +45:43:23.6
91.90196 -5.43885 galactic Cyg Second-epoch detections are separated by 7.6" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 1974206426561897856 | 21:42:11.99 +45:44:09.0 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 1974206426561897856,2461061.5558,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1974206426561897856 20260121.0558 13.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:42:11.28 +45:43:23.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.5558,13.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.0558 13.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:48:57.54 +47:58:58.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.56 21:56:06.56 +45:47:27.6
93.82366 -6.93892 galactic Cyg Second-epoch detections are separated by 4.3" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.0187+45.7903 | 21:56:08.60 +45:47:38.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.0187+45.7903,2461061.5558,13.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.0187+45.7903 20260121.0558 13.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:56:06.56 +45:47:27.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.46 21:10:44.96 +47:12:12.8
89.03304 -0.61522 galactic Cyg Second-epoch detections are separated by 8.7" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J317.7006+47.2110 | 21:10:44.96 +47:12:12.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J317.7006+47.2110,2461061.5558,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J317.7006+47.2110 20260121.0558 13.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:10:44.96 +47:12:12.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.48 21:37:16.72 +51:02:03.3
94.81093 -0.91806 galactic Cyg Second-epoch detections are separated by 8.5" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J324.3123+51.0313 | 21:37:16.72 +51:02:03.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J324.3123+51.0313,2461061.5558,13.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J324.3123+51.0313 20260121.0558 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:37:16.72 +51:02:03.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.46 20:57:25.60 +48:52:32.6
88.79365 2.15888 galactic Cyg Second-epoch detections are separated by 6.9" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2168573109960059392 | 20:57:26.83 +48:51:50.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2168573109960059392,2461061.5558,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2168573109960059392 20260121.0558 13.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:57:25.60 +48:52:32.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1975805803669616000,2461061.5558,13.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1975805803669616000 20260121.0558 13.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:08:32.85 +48:39:23.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.53 21:59:32.93 +48:20:21.7
95.86449 -5.28983 galactic Cyg Second-epoch detections are separated by 6.7" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1976197092370886016 | 21:59:28.21 +48:20:19.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1976197092370886016,2461061.5558,13.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1976197092370886016 20260121.0558 13.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:59:32.93 +48:20:21.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.57 22:12:59.93 +48:52:24.0
97.98485 -6.17106 galactic Lac Second-epoch detections are separated by 7.8" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J333.2392+48.8626 | 22:12:56.26 +48:52:28.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J333.2392+48.8626,2461061.5558,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J333.2392+48.8626 20260121.0558 13.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:12:59.93 +48:52:24.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.49 21:42:29.59 +51:09:32.7
95.50829 -1.36493 galactic Cyg Second-epoch detections are separated by 8.9" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1980828231038642688 | 21:42:28.46 +51:09:57.8 (Gaia DR3) | ROT (local) | (local) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1980828231038642688,2461061.5558,13.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1980828231038642688 20260121.0558 13.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:42:29.59 +51:09:32.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.61 21:14:02.67 +46:16:58.1
88.75115 -1.65782 galactic Cyg Second-epoch detections are separated by 5.9" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J318.5037+46.2779 | 21:14:02.67 +46:16:58.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.094+/- (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J318.5037+46.2779,2461061.5558,13.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J318.5037+46.2779 20260121.0558 13.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:14:02.67 +46:16:58.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.63 22:02:18.49 +48:07:24.3
96.10052 -5.73993 galactic Cyg Second-epoch detections are separated by 8.2" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1976150878521639040 | 22:02:20.09 +48:07:33.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1976150878521639040,2461061.5558,13.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1976150878521639040 20260121.0558 13.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:02:18.49 +48:07:24.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.57 21:41:56.74 +46:23:51.9
92.31525 -4.90282 galactic Cyg Second-epoch detections are separated by 8.9" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1977259907796687616 | 21:41:57.16 +46:23:46.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1977259907796687616,2461061.5558,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1977259907796687616 20260121.0558 13.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:41:56.74 +46:23:51.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.65 21:41:10.95 +45:49:27.0
91.83616 -5.24744 galactic Cyg Second-epoch detections are separated by 7.6" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.3097+45.8162 | 21:41:11.05 +45:49:11.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.3097+45.8162,2461061.5558,13.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.3097+45.8162 20260121.0558 13.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:41:10.95 +45:49:27.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.78 21:55:01.84 +50:24:55.4
96.56265 -3.20040 galactic Cyg Second-epoch detections are separated by 7.8" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1979808575756198784 | 21:54:58.59 +50:24:32.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1979808575756198784,2461061.5558,13.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1979808575756198784 20260121.0558 13.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:55:01.84 +50:24:55.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.5558,13.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.0558 13.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:38:05.10 +50:47:04.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1978879076114358528,2461061.5558,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1978879076114358528 20260121.0558 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:39:04.16 +49:02:36.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.66 21:58:57.88 +47:45:08.7
95.42693 -5.69521 galactic Cyg Second-epoch detections are separated by 8.7" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.7340+47.7572 | 21:58:56.04 +47:45:34.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.7340+47.7572,2461061.5558,13.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.7340+47.7572 20260121.0558 13.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:58:57.88 +47:45:08.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.66 21:49:49.32 +47:23:42.1
93.99264 -5.01253 galactic Cyg Second-epoch detections are separated by 7.9" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1974773774562807808 | 21:49:47.11 +47:24:20.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1974773774562807808,2461061.5558,13.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1974773774562807808 20260121.0558 13.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:49:49.32 +47:23:42.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.52 21:09:32.06 +46:47:18.7
88.58807 -0.74636 galactic Cyg Second-epoch detections are separated by 8.2" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J317.3798+46.7879 | 21:09:33.49 +46:47:26.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J317.3798+46.7879,2461061.5558,13.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J317.3798+46.7879 20260121.0558 13.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:09:32.06 +46:47:18.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.5558,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.0558 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:17:58.75 +46:29:02.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.61 21:38:51.74 +46:12:43.7
91.79120 -4.68998 galactic Cyg Second-epoch detections are separated by 6.6" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J324.7085+46.2126 | 21:38:48.88 +46:13:06.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J324.7085+46.2126,2461061.5558,13.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J324.7085+46.2126 20260121.0558 13.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:38:51.74 +46:12:43.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.75 22:15:49.07 +49:57:33.0
98.98272 -5.53557 galactic Lac Second-epoch detections are separated by 6.3" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J333.9768+49.9472 | 22:15:51.48 +49:57:14.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G4 1940AN....270..201M Cl* NGC 7243 M 91
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J333.9768+49.9472,2461061.5558,13.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J333.9768+49.9472 20260121.0558 13.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:15:49.07 +49:57:33.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.5558,13.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.0558 13.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:18:53.85 +50:00:26.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.5558,13.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.0558 13.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:51:14.77 +46:35:58.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.70 21:48:52.44 +47:56:32.6
94.21921 -4.48899 galactic Cyg Second-epoch detections are separated by 7.6" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J327.2164+47.9460 | 21:48:52.44 +47:56:32.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J327.2164+47.9460,2461061.5558,13.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J327.2164+47.9460 20260121.0558 13.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:48:52.44 +47:56:32.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.70 21:44:37.70 +45:52:31.3
92.32518 -5.60194 galactic Cyg Second-epoch detections are separated by 3.8" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J326.1505+45.8905 | 21:44:35.50 +45:53:05.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J326.1505+45.8905,2461061.5558,13.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J326.1505+45.8905 20260121.0558 13.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:44:37.70 +45:52:31.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.76 21:36:18.63 +50:55:05.4
94.61996 -0.90256 galactic Cyg Second-epoch detections are separated by 8.5" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J324.0741+50.9253 | 21:36:16.91 +50:55:35.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J324.0741+50.9253,2461061.5558,13.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J324.0741+50.9253 20260121.0558 13.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:36:18.63 +50:55:05.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.72 21:21:35.80 +50:50:31.1
92.88316 0.63855 galactic Cyg Second-epoch detections are separated by 7.9" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2171978606717301888 | 21:21:39.73 +50:50:16.1 (Gaia DR3) | S (local) | (local) | Gaia3var=NOT_AVAILABLE SpType: A0V 1939UppAn...1a...1V BD+50 3317
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2171978606717301888,2461061.5558,13.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2171978606717301888 20260121.0558 13.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:21:35.80 +50:50:31.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J211504.93+470021.2,2461061.5558,13.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J211504.93+470021.2 20260121.0558 13.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:15:02.85 +47:00:11.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1977362162385444864,2461061.5558,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1977362162385444864 20260121.0558 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:33:35.76 +45:51:25.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J220449.15+472429.5,2461061.5558,13.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J220449.15+472429.5 20260121.0558 13.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:04:51.23 +47:24:34.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.80 22:01:17.62 +50:36:33.2
97.47051 -3.65609 galactic Cyg Second-epoch detections are separated by 7.4" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J330.3185+50.6092 | 22:01:17.62 +50:36:33.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J330.3185+50.6092,2461061.5558,13.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J330.3185+50.6092 20260121.0558 13.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:01:17.62 +50:36:33.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.77 21:50:27.38 +47:11:52.0
93.95019 -5.23318 galactic Cyg Second-epoch detections are separated by 7.2" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1974720826204394880 | 21:50:28.54 +47:12:15.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1974720826204394880,2461061.5558,13.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1974720826204394880 20260121.0558 13.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:50:27.38 +47:11:52.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.79 22:15:52.92 +46:56:27.1
97.28064 -8.03640 galactic Lac Second-epoch detections are separated by 6.5" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ASASSN-V J221553.78+465558.1 | 22:15:53.78 +46:55:58.0 (Gaia DR3) | L (local) | (local) | Gaia3var=VARIABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J221553.78+465558.1,2461061.5558,13.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J221553.78+465558.1 20260121.0558 13.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:15:52.92 +46:56:27.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.79 22:12:40.62 +46:34:51.3
96.61797 -8.01995 galactic Lac Second-epoch detections are separated by 7.9" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1963344626072987776 | 22:12:38.86 +46:35:28.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1963344626072987776,2461061.5558,13.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1963344626072987776 20260121.0558 13.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:12:40.62 +46:34:51.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2000797702970763136,2461061.5558,13.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2000797702970763136 20260121.0558 13.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:13:24.08 +50:19:03.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.80 21:12:55.36 +47:41:48.9
89.64414 -0.54463 galactic Cyg Second-epoch detections are separated by 8.0" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ASASSN-V J211256.23+474222.1 | 21:12:56.23 +47:42:22.0 (Gaia DR3) | L (local) | (local) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J211256.23+474222.1,2461061.5558,13.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J211256.23+474222.1 20260121.0558 13.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:12:55.36 +47:41:48.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.76 21:53:06.49 +45:59:18.3
93.53730 -6.45849 galactic Cyg Second-epoch detections are separated by 8.6" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J328.2734+45.9781 | 21:53:08.32 +45:58:42.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J328.2734+45.9781,2461061.5558,13.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J328.2734+45.9781 20260121.0558 13.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:53:06.49 +45:59:18.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.78 21:14:50.64 +50:45:42.5
92.07852 1.34387 galactic Cyg Second-epoch detections are separated by 8.7" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2166205792705962240 | 21:14:46.24 +50:46:01.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: OB- 1964LS....C03....0H LS III +50 13
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2166205792705962240,2461061.5558,13.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2166205792705962240 20260121.0558 13.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:14:50.64 +50:45:42.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J213422.31+465148.9,2461061.5558,13.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J213422.31+465148.9 20260121.0558 13.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:34:24.47 +46:51:43.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.75 21:14:18.50 +46:33:09.1
88.97770 -1.50441 galactic Cyg Second-epoch detections are separated by 7.1" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J318.5747+46.5633 | 21:14:20.56 +46:33:39.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J318.5747+46.5633,2461061.5558,13.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J318.5747+46.5633 20260121.0558 13.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:14:18.50 +46:33:09.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.82 21:40:45.00 +46:04:21.6
91.94414 -5.01114 galactic Cyg Second-epoch detections are separated by 4.2" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1977230633298683520 | 21:40:46.31 +46:04:32.0 (Gaia DR3) | ROT (local) | (local) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1977230633298683520,2461061.5558,13.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1977230633298683520 20260121.0558 13.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:40:45.00 +46:04:21.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.86 22:04:42.10 +49:30:55.5
97.25352 -4.85970 galactic Lac Second-epoch detections are separated by 8.8" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J331.1890+49.5073 | 22:04:42.10 +49:30:55.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J331.1890+49.5073,2461061.5558,13.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J331.1890+49.5073 20260121.0558 13.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:04:42.10 +49:30:55.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1999716741295835648,2461061.5558,14.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1999716741295835648 20260121.0558 14.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:20:34.55 +49:21:51.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.90 21:45:33.96 +49:24:08.8
94.73933 -3.01910 galactic Cyg Second-epoch detections are separated by 8.4" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 1978195970150391680 | 21:45:35.23 +49:23:36.7 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 1978195970150391680,2461061.5558,13.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1978195970150391680 20260121.0558 13.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:45:33.96 +49:24:08.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 14.03 22:01:28.74 +50:31:49.9
97.44652 -3.73662 galactic Cyg Second-epoch detections are separated by 6.8" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1979954157965825280 | 22:01:25.83 +50:31:32.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1979954157965825280,2461061.5558,14.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1979954157965825280 20260121.0558 14.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:01:28.74 +50:31:49.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.86 22:03:38.54 +47:28:59.6
95.89430 -6.38645 galactic Lac Second-epoch detections are separated by 7.9" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J330.9269+47.4716 | 22:03:39.74 +47:28:32.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J330.9269+47.4716,2461061.5558,13.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J330.9269+47.4716 20260121.0558 13.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:03:38.54 +47:28:59.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 14.04 22:21:02.18 +49:26:02.7
99.39658 -6.44022 galactic Lac Second-epoch detections are separated by 5.8" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J335.2472+49.4358 | 22:21:02.18 +49:26:02.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J335.2472+49.4358,2461061.5558,14.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J335.2472+49.4358 20260121.0558 14.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:21:02.18 +49:26:02.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1972287160311536768,2461061.5558,13.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1972287160311536768 20260121.0558 13.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:28:31.18 +47:04:23.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.98 21:57:01.47 +47:15:35.1
94.86290 -5.88276 galactic Cyg Second-epoch detections are separated by 7.4" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.2583+47.2547 | 21:57:01.37 +47:15:10.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.2583+47.2547,2461061.5558,13.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.2583+47.2547 20260121.0558 13.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:57:01.47 +47:15:35.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.88 22:01:12.47 +48:34:18.9
96.22577 -5.27192 galactic Cyg Second-epoch detections are separated by 7.5" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J330.2835+48.5637 | 22:01:08.34 +48:34:01.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J330.2835+48.5637,2461061.5558,13.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J330.2835+48.5637 20260121.0558 13.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:01:12.47 +48:34:18.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 14.11 22:18:36.00 +49:09:45.9
98.91257 -6.44823 galactic Lac Second-epoch detections are separated by 8.8" and 8.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J334.6594+49.1650 | 22:18:36.00 +49:09:45.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J334.6594+49.1650,2461061.5558,14.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J334.6594+49.1650 20260121.0558 14.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:18:36.00 +49:09:45.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 14.08 21:53:14.86 +46:33:54.4
93.92064 -6.02495 galactic Cyg Second-epoch detections are separated by 8.6" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1974464296398760576 | 21:53:11.90 +46:34:21.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1974464296398760576,2461061.5558,14.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1974464296398760576 20260121.0558 14.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:53:14.86 +46:33:54.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 14.06 22:16:26.44 +49:41:22.3
98.91436 -5.81516 galactic Lac Second-epoch detections are separated by 7.9" and 9.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1999961661816936576 | 22:16:28.59 +49:40:50.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.323+/-0.144 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1999961661816936576,2461061.5558,14.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1999961661816936576 20260121.0558 14.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:16:26.44 +49:41:22.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.5558,13.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.0558 13.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:58:02.28 +49:08:27.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.5558,14.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.0558 14.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:45:05.77 +45:49:54.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.90 21:38:43.16 +50:33:26.9
94.66369 -1.42548 galactic Cyg Second-epoch detections are separated by 7.7" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1979283589000719616 | 21:38:40.68 +50:32:59.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1979283589000719616,2461061.5558,13.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1979283589000719616 20260121.0558 13.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:38:43.16 +50:33:26.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.89 21:41:24.47 +50:53:17.0
95.20171 -1.45793 galactic Cyg Second-epoch detections are separated by 7.1" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.3466+50.9096 | 21:41:23.85 +50:53:54.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.3466+50.9096,2461061.5558,13.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.3466+50.9096 20260121.0558 13.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:41:24.47 +50:53:17.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 14.00 22:11:47.25 +46:35:01.4
96.49337 -7.92974 galactic Lac Second-epoch detections are separated by 6.1" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J332.9474+46.5964 | 22:11:47.25 +46:35:01.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J332.9474+46.5964,2461061.5558,14.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J332.9474+46.5964 20260121.0558 14.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:11:47.25 +46:35:01.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 14.08 21:59:42.92 +48:11:04.5
95.79188 -5.42946 galactic Cyg Second-epoch detections are separated by 5.8" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.9150+48.1880 | 21:59:42.92 +48:11:04.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.9150+48.1880,2461061.5558,14.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.9150+48.1880 20260121.0558 14.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:59:42.92 +48:11:04.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 14.10 21:57:36.75 +48:35:44.8
95.76710 -4.89063 galactic Cyg Second-epoch detections are separated by 4.1" and 9.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.4178+48.5899 | 21:57:37.79 +48:35:10.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.4178+48.5899,2461061.5558,14.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.4178+48.5899 20260121.0558 14.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:57:36.75 +48:35:44.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 14.07 22:16:48.60 +46:04:13.4
96.91817 -8.84552 galactic Lac Second-epoch detections are separated by 7.1" and 9.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J334.2061+46.0900 | 22:16:48.36 +46:04:56.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J334.2061+46.0900,2461061.5558,14.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J334.2061+46.0900 20260121.0558 14.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:16:48.60 +46:04:13.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.97 21:31:29.19 +45:28:16.3
90.33855 -4.37063 galactic Cyg Second-epoch detections are separated by 4.2" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J322.8840+45.4608 | 21:31:30.07 +45:27:42.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J322.8840+45.4608,2461061.5558,13.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J322.8840+45.4608 20260121.0558 13.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:31:29.19 +45:28:16.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 14.12 22:14:45.87 +47:02:14.6
97.17715 -7.84898 galactic Lac Second-epoch detections are separated by 7.4" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ASASSN-V J221441.58+470224.8 | 22:14:41.58 +47:02:24.7 (Gaia DR3) | L (local) | (local) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J221441.58+470224.8,2461061.5558,14.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J221441.58+470224.8 20260121.0558 14.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:14:45.87 +47:02:14.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 14.12 22:16:29.51 +46:25:17.3
97.07208 -8.52437 galactic Lac Second-epoch detections are separated by 8.3" and 9.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J334.1102+46.4246 | 22:16:29.51 +46:25:17.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J334.1102+46.4246,2461061.5558,14.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J334.1102+46.4246 20260121.0558 14.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:16:29.51 +46:25:17.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 13.96 22:12:28.77 +47:41:33.8
97.23361 -7.09001 galactic Lac Second-epoch detections are separated by 7.4" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1975551541600364288 | 22:12:30.88 +47:42:08.0 (Gaia DR3) | ROT (local) | (local) | Gaia3var=VARIABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1975551541600364288,2461061.5558,13.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1975551541600364288 20260121.0558 13.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:12:28.77 +47:41:33.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.5558,14.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.0558 14.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:57:05.66 +45:38:57.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 14.10 22:12:35.82 +47:01:30.1
96.86391 -7.64839 galactic Lac Second-epoch detections are separated by 5.3" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J333.1566+47.0152 | 22:12:35.82 +47:01:30.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J333.1566+47.0152,2461061.5558,14.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J333.1566+47.0152 20260121.0558 14.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:12:35.82 +47:01:30.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1963408397746524160,2461061.5558,14.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1963408397746524160 20260121.0558 14.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:12:32.23 +46:59:32.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 14.11 22:17:55.14 +46:18:05.7
97.21019 -8.76176 galactic Lac Second-epoch detections are separated by 8.1" and 9.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J334.4732+46.2827 | 22:17:54.75 +46:17:21.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J334.4732+46.2827,2461061.5558,14.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J334.4732+46.2827 20260121.0558 14.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:17:55.14 +46:18:05.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 14.08 22:06:56.40 +47:17:19.0
96.22991 -6.87461 galactic Lac Second-epoch detections are separated by 8.1" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J331.7464+47.2837 | 22:06:56.22 +47:17:02.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.479+/-0.044 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J331.7464+47.2837,2461061.5558,14.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J331.7464+47.2837 20260121.0558 14.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:06:56.40 +47:17:19.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1974227970126512896,2461061.5558,14.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1974227970126512896 20260121.0558 14.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:41:05.61 +46:02:22.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1976015844745958016,2461061.5558,14.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1976015844745958016 20260121.0558 14.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:57:47.98 +47:31:54.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1963421626245746432,2461061.5558,14.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1963421626245746432 20260121.0558 14.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:12:08.81 +47:04:58.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 14.10 21:38:08.45 +50:49:15.0
94.77014 -1.16774 galactic Cyg Second-epoch detections are separated by 7.7" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J324.5287+50.8301 | 21:38:08.45 +50:49:15.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J324.5287+50.8301,2461061.5558,14.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J324.5287+50.8301 20260121.0558 14.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:38:08.45 +50:49:15.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1976110334029736832,2461061.5558,14.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1976110334029736832 20260121.0558 14.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:01:00.27 +47:48:36.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1976023335169392768,2461061.5558,14.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1976023335169392768 20260121.0558 14.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:58:53.76 +47:38:22.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1974480548555995648,2461061.5558,14.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1974480548555995648 20260121.0558 14.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:51:25.03 +46:24:44.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.5558,14.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.0558 14.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:17:17.07 +50:16:47.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 14.18 22:01:47.11 +49:54:47.4
97.11304 -4.25899 galactic Cyg Second-epoch detections are separated by 8.6" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1976900917253798272 | 22:01:47.31 +49:55:11.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1976900917253798272,2461061.5558,14.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1976900917253798272 20260121.0558 14.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:01:47.11 +49:54:47.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 14.23 22:17:37.31 +49:34:09.4
99.00641 -6.02170 galactic Lac Second-epoch detections are separated by 6.3" and 9.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1999921323482439168 | 22:17:34.65 +49:33:50.5 (Gaia DR3) | ROT (local) | (local) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1999921323482439168,2461061.5558,14.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1999921323482439168 20260121.0558 14.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:17:37.31 +49:34:09.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.5558,14.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.0558 14.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:40:41.60 +49:58:49.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1974208896159550080,2461061.5558,14.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1974208896159550080 20260121.0558 14.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:41:48.15 +45:46:11.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 14.15 21:36:44.40 +45:32:15.3
91.06313 -4.94521 galactic Cyg Second-epoch detections are separated by 7.3" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1977109098596849664 | 21:36:41.37 +45:31:48.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1977109098596849664,2461061.5558,14.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1977109098596849664 20260121.0558 14.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:36:44.40 +45:32:15.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 14.27 22:16:39.77 +46:03:38.2
96.89124 -8.83923 galactic Lac Second-epoch detections are separated by 6.5" and 8.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J334.1623+46.0503 | 22:16:37.94 +46:03:08.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J334.1623+46.0503,2461061.5558,14.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J334.1623+46.0503 20260121.0558 14.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:16:39.77 +46:03:38.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J221353.08+471154.3,2461061.5558,14.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J221353.08+471154.3 20260121.0558 14.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:13:51.58 +47:11:40.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 14.23 21:53:23.93 +46:11:02.0
93.70033 -6.33806 galactic Cyg Second-epoch detections are separated by 8.9" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1974418494867156224 | 21:53:23.59 +46:10:38.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1974418494867156224,2461061.5558,14.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1974418494867156224 20260121.0558 14.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:53:23.93 +46:11:02.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 14.28 22:12:32.92 +46:23:00.9
96.48524 -8.16881 galactic Lac Second-epoch detections are separated by 3.5" and 9.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J333.1323+46.3865 | 22:12:32.82 +46:23:33.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J333.1323+46.3865,2461061.5558,14.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J333.1323+46.3865 20260121.0558 14.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:12:32.92 +46:23:00.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 14.22 21:37:47.08 +47:24:21.0
92.45049 -3.67679 galactic Cyg Second-epoch detections are separated by 7.9" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1977608281186813696 | 21:37:50.07 +47:24:08.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1977608281186813696,2461061.5558,14.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1977608281186813696 20260121.0558 14.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:37:47.08 +47:24:21.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 14.29 22:14:38.42 +49:44:44.9
98.70439 -5.60492 galactic Lac Second-epoch detections are separated by 7.9" and 8.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J333.6504+49.7468 | 22:14:38.42 +49:44:44.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J333.6504+49.7468,2461061.5558,14.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J333.6504+49.7468 20260121.0558 14.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:14:38.42 +49:44:44.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1979566404008517120,2461061.5558,14.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1979566404008517120 20260121.0558 14.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:53:39.79 +49:42:09.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 14.30 22:12:34.30 +50:21:13.4
98.77667 -4.91597 galactic Lac Second-epoch detections are separated by 7.9" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2000801448184555008 | 22:12:37.02 +50:20:40.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A2 1956PMcCO..13a....B AG+50 1763
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2000801448184555008,2461061.5558,14.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2000801448184555008 20260121.0558 14.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:12:34.30 +50:21:13.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 14.33 22:07:03.66 +50:24:19.3
98.08787 -4.36539 galactic Lac Second-epoch detections are separated by 8.4" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J331.7662+50.3998 | 22:07:03.66 +50:24:19.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J331.7662+50.3998,2461061.5558,14.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J331.7662+50.3998 20260121.0558 14.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:07:03.66 +50:24:19.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1978043825227270656,2461061.5558,14.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1978043825227270656 20260121.0558 14.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:42:33.25 +48:29:50.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 14.25 21:39:13.95 +46:06:50.6
91.77383 -4.80587 galactic Cyg Second-epoch detections are separated by 4.1" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J324.7983+46.1150 | 21:39:13.95 +46:06:50.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J324.7983+46.1150,2461061.5558,14.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J324.7983+46.1150 20260121.0558 14.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:39:13.95 +46:06:50.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 14.46 22:16:54.22 +49:57:05.3
99.12378 -5.63975 galactic Lac Second-epoch detections are separated by 8.9" and 9.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J334.2447+49.9560 | 22:16:54.22 +49:57:05.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J334.2447+49.9560,2461061.5558,14.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J334.2447+49.9560 20260121.0558 14.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:16:54.22 +49:57:05.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 14.36 21:35:35.67 +48:42:18.8
93.04938 -2.46654 galactic Cyg Second-epoch detections are separated by 8.4" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J323.9091+48.7029 | 21:35:35.67 +48:42:18.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J323.9091+48.7029,2461061.5558,14.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J323.9091+48.7029 20260121.0558 14.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:35:35.67 +48:42:18.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 14.41 22:06:03.60 +48:27:44.6
96.80719 -5.84003 galactic Lac Second-epoch detections are separated by 7.8" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1975777697402557568 | 22:06:04.80 +48:27:07.6 (Gaia DR3) | ROT (local) | (local) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1975777697402557568,2461061.5558,14.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1975777697402557568 20260121.0558 14.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:06:03.60 +48:27:44.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 14.40 22:01:46.28 +50:40:30.1
97.57080 -3.64916 galactic Cyg Second-epoch detections are separated by 8.8" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J330.4512+50.6632 | 22:01:46.28 +50:40:30.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J330.4512+50.6632,2461061.5558,14.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J330.4512+50.6632 20260121.0558 14.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:01:46.28 +50:40:30.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 14.26 22:14:00.75 +48:44:17.3
98.04546 -6.37722 galactic Lac Second-epoch detections are separated by 7.4" and 8.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J333.5014+48.7395 | 22:14:00.75 +48:44:17.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J333.5014+48.7395,2461061.5558,14.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J333.5014+48.7395 20260121.0558 14.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:14:00.75 +48:44:17.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1980534253427684608,2461061.5558,14.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1980534253427684608 20260121.0558 14.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:45:03.17 +50:18:26.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1979432263597419008,2461061.5558,14.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1979432263597419008 20260121.0558 14.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:51:18.40 +49:07:02.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 14.24 21:42:50.97 +50:33:43.6
95.16080 -1.85369 galactic Cyg Second-epoch detections are separated by 7.6" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.6908+50.5626 | 21:42:47.46 +50:33:23.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.6908+50.5626,2461061.5558,14.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.6908+50.5626 20260121.0558 14.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:42:50.97 +50:33:43.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1978666939091757440,2461061.5558,14.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1978666939091757440 20260121.0558 14.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:34:25.29 +48:42:57.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 14.48 22:01:26.16 +48:48:20.8
96.39776 -5.10830 galactic Cyg Second-epoch detections are separated by 7.9" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J330.3596+48.7957 | 22:01:26.16 +48:48:20.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J330.3596+48.7957,2461061.5558,14.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J330.3596+48.7957 20260121.0558 14.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:01:26.16 +48:48:20.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.5558,14.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.0558 14.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:45:40.26 +49:24:07.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 14.45 22:00:39.35 +48:52:44.2
96.33955 -4.97240 galactic Cyg Second-epoch detections are separated by 6.5" and 9.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J330.1499+48.8846 | 22:00:39.35 +48:52:44.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J330.1499+48.8846,2461061.5558,14.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J330.1499+48.8846 20260121.0558 14.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:00:39.35 +48:52:44.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J221054.20+481626.7,2461061.5558,14.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J221054.20+481626.7 20260121.0558 14.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:10:55.80 +48:16:24.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.5558,14.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.0558 14.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:58:09.13 +47:34:37.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.5558,14.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.0558 14.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:01:45.21 +48:22:58.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1976432594018829824,2461061.5558,14.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1976432594018829824 20260121.0558 14.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:00:24.00 +48:57:36.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 14.39 21:08:58.80 +46:27:43.7
88.28384 -0.89820 galactic Cyg Second-epoch detections are separated by 8.2" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J317.2381+46.4629 | 21:08:58.80 +46:27:43.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J317.2381+46.4629,2461061.5558,14.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J317.2381+46.4629 20260121.0558 14.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:08:58.80 +46:27:43.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.5558,14.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.0558 14.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:03:50.67 +49:37:59.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2171904630198257792,2461061.5558,14.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2171904630198257792 20260121.0558 14.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:21:58.91 +50:25:29.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 14.48 21:01:15.37 +45:15:10.9
86.48530 -0.70853 galactic Cyg Second-epoch detections are separated by 4.9" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.3194+45.2417 | 21:01:15.37 +45:15:10.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.3194+45.2417,2461061.5558,14.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.3194+45.2417 20260121.0558 14.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:15.37 +45:15:10.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 14.44 22:15:45.15 +46:18:13.9
96.89849 -8.54949 galactic Lac Second-epoch detections are separated by 3.8" and 8.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1963218560189805184 | 22:15:45.60 +46:17:39.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1963218560189805184,2461061.5558,14.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1963218560189805184 20260121.0558 14.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:15:45.15 +46:18:13.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 14.36 21:56:13.54 +48:46:18.2
95.69499 -4.61101 galactic Cyg Second-epoch detections are separated by 8.9" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.0485+48.7721 | 21:56:12.82 +48:46:43.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.0485+48.7721,2461061.5558,14.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.0485+48.7721 20260121.0558 14.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:56:13.54 +48:46:18.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.5558,14.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.0558 14.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:27:00.86 +49:45:02.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.5558,14.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.0558 14.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:40:59.02 +46:00:23.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.5558,14.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.0558 14.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:28:05.69 +45:30:23.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 14.42 21:24:31.33 +50:25:38.5
92.92227 0.01762 galactic Cyg Second-epoch detections are separated by 7.9" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2171247152294681472 | 21:24:32.94 +50:26:12.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2171247152294681472,2461061.5558,14.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2171247152294681472 20260121.0558 14.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:24:31.33 +50:25:38.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0558 2461061.5558 14.47 21:42:24.30 +45:43:18.1
91.92963 -5.46489 galactic Cyg Second-epoch detections are separated by 3.4" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.5937+45.7214 | 21:42:24.30 +45:43:18.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.5937+45.7214,2461061.5558,14.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.5937+45.7214 20260121.0558 14.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:42:24.30 +45:43:18.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0410 Cyg,2461061.5558,10.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0410 Cyg 20260121.0558 10.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:40:48.89 +49:49:40.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0667 Cyg,2461061.5558,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0667 Cyg 20260121.0558 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:49:25.85 +49:33:12.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Processing complete!
Total number of candidates identified: 306
Processing log:
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.59461456 23.12.2025 02:16:04.698 /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits
First image: 2461032.59461456 23.12.2025 02:16:04.698 /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits
Last image: 2461061.55605506 21.01.2026 01:20:33.157 /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 50
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.90
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 106 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 33925
Objects passed selection criteria: 33903
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 32638.2
Average stars matched: 31820.5 (97.4945 %)
Memory usage VmPeak: 132628 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Jan 14 09:05:05 CST 2026
VaST build number 1.0rc88-183-g45c3f81a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-01-14)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Jan 21 01:25:22 CST 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.59461456 23.12.2025 02:16:04.698 /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits
First image: 2461032.59461456 23.12.2025 02:16:04.698 /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits
Last image: 2461061.55605506 21.01.2026 01:20:33.157 /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 1464
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.57
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 1035 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 2.1 # or , in mag.arcsec-2
ANALYSIS_THRESH 2.1 # or , in mag.arcsec-2
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 263911
Objects passed selection criteria: 263314
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 251681
Average stars matched: 241314 (95.881 %)
Memory usage VmPeak: 2016748 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Jan 14 09:05:05 CST 2026
VaST build number 1.0rc88-183-g45c3f81a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-01-14)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Jan 21 01:52:46 CST 2026
Host name: tau
############################################################
Filtering log:
######## Processing parameters ########
AAVSO_COMMENT_STRING= NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
ASTCHECK_ASTEROID_SEARCH_RADIUS_ARCSEC=
BAD_REGION_FILE= /var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst
CAMERA_SETTINGS= TTUQ1b1x1
CHECK_POINTING_ACCURACY= yes
DARK_FRAMES_DIR= /var/www/nmw_calibration/TTUQ1b1x1/darks
EXCLUSION_LIST= ../exclusion_list_TTUQ1.txt
FILTER_BAD_IMG__MAX_APERTURE_STAR_SIZE_PIX= 12.5
FILTER_BAD_IMG__MAX_ELONGATION_AminusB_PIX= 0.55
FILTER_BAD_IMG__MIN_APERTURE_STAR_SIZE_PIX= 2.0
FILTER_BRIGHT_MAG_CUTOFF_TRANSIENT_SEARCH= -5
FILTER_FAINT_MAG_CUTOFF_TRANSIENT_SEARCH= 14.5
FLAT_FIELD_FILE= /var/www/nmw_calibration/TTUQ1b1x1/flats/mff_TTUQ1b1x1_2025-12-22.fit
FRAME_EDGE_OFFSET_PIX= 25
GAIA_BAND_FOR_CATALOGED_SOURCE_CHECK=
MAX_NEW_TO_REF_MEAN_IMG_VALUE_RATIO= 100
MAX_NEW_IMG_MEAN_VALUE= 25000
MAX_SD_RATIO_OF_SECOND_EPOCH_IMGS= 0.18
MAX_SD_RATIO_OF_SECOND_EPOCH_IMGS_SOFT_LIMIT= 0.12
MPC_CODE= 500
NMW_CALIBRATION= /var/www/nmw_calibration
NUMBER_OF_DETECTED_TRANSIENTS_BEFORE_FILTERING_HARD_LIMIT= 3000
NUMBER_OF_DETECTED_TRANSIENTS_BEFORE_FILTERING_SOFT_LIMIT= 2000
OMP_NUM_THREADS=
ONLINE_MPCHECKER_BUTTON_ASTEROID_SEARCH_RADIUS_ARCMIN=
PHOTOMETRIC_CALIBRATION=
REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES= yes
SEXTRACTOR_CONFIG_BRIGHTSTARPASS= default.sex.telephoto_lens_onlybrightstars_v1
SEXTRACTOR_CONFIG_FILES= default.sex.telephoto_lens_onlybrightstars_v1 default.sex.telephoto_lens_vSTL
STARMATCH_RADIUS_PIX= 3.5
SYSREM_ITERATIONS= 0
TELESCOP=
TELESCOP_NAME_KNOWN_TO_VaST_FOR_FOV_DETERMINATION=
UCAC5_PLATESOLVE_ITERATIONS= 2
FPACK_FULLY_CALIBRATED_IMAGE= no
#######################################
HOSTNAME= tau
USER=
HOME=
#######################################
Reference image directory is set to /mnt/usb2/NMW-TexasTech/reference_imgs
VIZIER_SITE=vizier.china-vo.org
INFO: MAKE_PNG_PLOTS is set to yes
FITS_FILE_EXT=fits
CALIBRATION_STATUS_PREFIX=
Fields in the data directory:
Cyg-04-Q1b1x1
#######################################
########### Starting Cyg-04-Q1b1x1 ###########
Processing Cyg-04-Q1b1x1
server tau has sufficient free disk space available: 185898 MB at /mnt/usb2/NMW-TexasTech/workdir
server tau has sufficient free disk space available: 185898 MB at .
Checking input images (2 new)
REFERENCE_EPOCH__FIRST_IMAGE= /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits
REFERENCE_EPOCH__SECOND_IMAGE= /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits
Small preview (one of the new images):
Large previews of the second-epoch (new) images:
MAKE_PNG_PLOTS=yes
renamed 'Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png' -> 'transient_report/Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits_preview.png'
Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits
renamed 'Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png' -> 'transient_report/Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits_preview.png'
Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits
Read-check the input FITS images... read-check OK
Blank image check the input FITS images... blank-image-check OK
Read date check the input FITS images... read-date-check OK
Mean value check the input FITS images... OK, at least two new images have mean values below the threshold.
----------------------------------------------
INFO: REFERENCE_EPOCH__FIRST_IMAGE_MEAN_VALUE= 733.3176
INFO: REFERENCE_EPOCH__FIRST_IMAGE_SD= 927.1301
INFO: SECOND_EPOCH__FIRST_IMAGE_MEAN_VALUE= 1412.1238
INFO: SECOND_EPOCH__FIRST_IMAGE_SD= 951.4298
INFO: SECOND_EPOCH__SECOND_IMAGE_MEAN_VALUE= 1396.5757
INFO: SECOND_EPOCH__SECOND_IMAGE_SD= 952.6875
----------------------------------------------
INFO: ref_to_second_epoch_img_mean_ratio= 1.92566
INFO: SECOND_EPOCH__SD_ratio= 0.001
----------------------------------------------
Calibration settings: DARK_FRAMES_DIR=/var/www/nmw_calibration/TTUQ1b1x1/darks FLAT_FIELD_FILE=/var/www/nmw_calibration/TTUQ1b1x1/flats/mff_TTUQ1b1x1_2025-12-22.fit
EXPTIME = 20.0 / [s] Exposure duration
SET-TEMP= -15.0 / [degC] CCD temperature setpoint
CCD-TEMP= -14.9 / [degC] CCD temperature
Exploring image header: /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits
CCD-TEMP= -14.900000 for /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits
SET-TEMP= -15.000000 for /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits
Header: 61 keys total, 10 keys left
Record 0: "" status=0
Record 1: "SIMPLE = T / C# FITS" status=0
Record 2: "BITPIX = 16" status=0
Record 3: "NAXIS = 2 / Dimensionality" status=0
Record 4: "NAXIS1 = 9576" status=0
Record 5: "NAXIS2 = 6388" status=0
Record 6: "BZERO = 32768" status=0
Record 7: "EXTEND = T / Extensions are permitted" status=0
Record 8: "IMAGETYP= 'LIGHT' / Type of exposure" status=0
Record 9: "EXPOSURE= 20.0 / [s] Exposure duration" status=0
Record 10: "EXPTIME = 20.0 / [s] Exposure duration" status=0
Record 11: "DATE-LOC= '2026-01-20T19:19:50.1136094' / Time of observation (local)" status=0
Record 12: "DATE-OBS= '2026-01-21T01:19:50.1136094' / Time of observation (UTC)" status=0
Record 13: "MJD-OBS = 61061.0554411225 / Modified Julian Date of observation" status=0
Record 14: "DATE-AVG= '2026-01-21T01:20:00.0151825' / Averaged midpoint time (UTC)" status=0
Record 15: "MJD-AVG = 61061.0555557292 / Modified Julian Date of averaged midpoint" status=0
Record 16: "XBINNING= 1 / X axis binning factor" status=0
Record 17: "YBINNING= 1 / Y axis binning factor" status=0
Record 18: "GAIN = 30 / Sensor gain" status=0
Record 19: "OFFSET = 30 / Sensor gain offset" status=0
Record 20: "XPIXSZ = 3.76 / [um] Pixel X axis size" status=0
Record 21: "YPIXSZ = 3.76 / [um] Pixel Y axis size" status=0
Record 22: "INSTRUME= 'QHY600M' / Imaging instrument name" status=0
Record 23: "CAMERAID= 'QHY600M-33d3d743814b8b447' / Imaging instrument identifier" status=0
Record 24: "SET-TEMP= -15.0 / [degC] CCD temperature setpoint" status=0
Record 25: "CCD-TEMP= -14.9 / [degC] CCD temperature" status=0
Record 26: "READOUTM= '2CMS-0' / Sensor readout mode" status=0
Record 27: "USBLIMIT= 50 / Camera-specific USB setting" status=0
Record 28: "TELESCOP= 'QHY600M-TTU1' / Name of telescope" status=0
Record 29: "FOCALLEN= 135.0 / [mm] Focal length" status=0
Record 30: "FOCRATIO= 2.2 / Focal ratio" status=0
Record 31: "RA = 323.999919737064 / [deg] RA of telescope" status=0
Record 32: "DEC = 45.9995018758798 / [deg] Declination of telescope" status=0
Record 33: "CENTALT = 33.8219444444444 / [deg] Altitude of telescope" status=0
Record 34: "CENTAZ = 306.566944444444 / [deg] Azimuth of telescope" status=0
Record 35: "AIRMASS = 1.79276039379112 / Airmass at frame center (Gueymard 1993)" status=0
Record 36: "PIERSIDE= 'East' / Telescope pointing state" status=0
Record 37: "SITEELEV= 1013.0 / [m] Observation site elevation" status=0
Record 38: "SITELAT = 33.748239 / [deg] Observation site latitude" status=0
Record 39: "SITELONG= -101.958391 / [deg] Observation site longitude" status=0
Record 40: "OBSERVER= 'Sokolovsky' / Observer name" status=0
Record 41: "OBSERVAT= 'TTU Skyview' / Observatory name" status=0
Record 42: "SITENAME= '' / Observatory site name" status=0
Record 43: "FWHEEL = 'Simulator' / Filter Wheel name" status=0
Record 44: "FILTER = 'CV' / Active filter name" status=0
Record 45: "OBJECT = 'Cyg-04' / Name of the object of interest" status=0
Record 46: "OBJCTRA = '21 36 00' / [H M S] RA of imaged object" status=0
Record 47: "OBJCTDEC= '+46 00 00' / [D M S] Declination of imaged object" status=0
Record 48: "OBJCTROT= 0.0 / [deg] planned rotation of imaged object" status=0
Record 49: "ROWORDER= 'TOP-DOWN' / FITS Image Orientation" status=0
Record 50: "EQUINOX = 2000.0 / Equinox of celestial coordinate system" status=0
Record 51: "SWCREATE= 'N.I.N.A. 3.2.0.9001 (x64)' / Software that created this file" status=0
Record 52: "QHY_EXP = 20.000096 / [s] Actual exposure time" status=0
Record 53: "QHY_PP = 13888.0 / [ps] pixelPeriod" status=0
Record 54: "QHY_LP = 85000.0 / [ns] linePeriod" status=0
Record 55: "GPS_LP = 85000.0 / [ns] linePeriod" status=0
Record 56: "QHY_FP = 20000160.0 / [us] framePeriod" status=0
Record 57: "QHY_CPL = 6120.0 / clocksPerLine" status=0
Record 58: "QHY_LPF = 235295.0 / linesPerFrame" status=0
Record 59: "QHY_AET = 20000096.0 / [us] actualExposureTime" status=0
Record 60: "QHY_LEM = T / isLongExposureMode" status=0
Record 61: "QHY_OFF0= 3767.777 / [us] RollingShutterEndOffset row 0" status=0
Allocating memory for image, dark and result arrays...
Reading image /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits 9576 6388 16 bitpix
SET-TEMP= -15.000000 for /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits
SET-TEMP= -15.000000 for /var/www/nmw_calibration/TTUQ1b1x1/darks/mdark_TTUQ1b1x1_-15C_20s_2026-01-08.fit
CCD-TEMP= -14.900000 for /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits
CCD-TEMP= -15.000000 for /var/www/nmw_calibration/TTUQ1b1x1/darks/mdark_TTUQ1b1x1_-15C_20s_2026-01-08.fit
Reading dark frame /var/www/nmw_calibration/TTUQ1b1x1/darks/mdark_TTUQ1b1x1_-15C_20s_2026-01-08.fit 9576 6388 16 bitpix
Dark frame is subtracted, output is written to /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/d_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits :)
Spent 0.582087 seconds
renamed 'mdark_TTUQ1b1x1_-15C_20s_2026-01-08.png' -> 'transient_report/dark.png'
MegaDivider v7
Reading image /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/d_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits 9576 6388 16 bitpix
Reading flat /var/www/nmw_calibration/TTUQ1b1x1/flats/mff_TTUQ1b1x1_2025-12-22.fit 9576 6388 16 bitpix
Avarage count on flat field image: 38918.354428
Minimal real count (from overscan): 5
Output is written to /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits :)
No overscan detected - all values seem high! (left_median=27736.5, right_median=26453.5)
renamed 'mff_TTUQ1b1x1_2025-12-22.png' -> 'transient_report/flat.png'
Using calibrated image CALIBRATED_SECOND_EPOCH__FIRST_IMAGE=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits
EXPTIME = 20.0 / [s] Exposure duration
SET-TEMP= -15.0 / [degC] CCD temperature setpoint
CCD-TEMP= -15.0 / [degC] CCD temperature
Exploring image header: /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits
CCD-TEMP= -15.000000 for /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits
SET-TEMP= -15.000000 for /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits
Header: 61 keys total, 10 keys left
Record 0: "" status=0
Record 1: "SIMPLE = T / C# FITS" status=0
Record 2: "BITPIX = 16" status=0
Record 3: "NAXIS = 2 / Dimensionality" status=0
Record 4: "NAXIS1 = 9576" status=0
Record 5: "NAXIS2 = 6388" status=0
Record 6: "BZERO = 32768" status=0
Record 7: "EXTEND = T / Extensions are permitted" status=0
Record 8: "IMAGETYP= 'LIGHT' / Type of exposure" status=0
Record 9: "EXPOSURE= 20.0 / [s] Exposure duration" status=0
Record 10: "EXPTIME = 20.0 / [s] Exposure duration" status=0
Record 11: "DATE-LOC= '2026-01-20T19:20:33.1570681' / Time of observation (local)" status=0
Record 12: "DATE-OBS= '2026-01-21T01:20:33.1570681' / Time of observation (UTC)" status=0
Record 13: "MJD-OBS = 61061.0559393172 / Modified Julian Date of observation" status=0
Record 14: "DATE-AVG= '2026-01-21T01:20:43.0904758' / Averaged midpoint time (UTC)" status=0
Record 15: "MJD-AVG = 61061.0560542825 / Modified Julian Date of averaged midpoint" status=0
Record 16: "XBINNING= 1 / X axis binning factor" status=0
Record 17: "YBINNING= 1 / Y axis binning factor" status=0
Record 18: "GAIN = 30 / Sensor gain" status=0
Record 19: "OFFSET = 30 / Sensor gain offset" status=0
Record 20: "XPIXSZ = 3.76 / [um] Pixel X axis size" status=0
Record 21: "YPIXSZ = 3.76 / [um] Pixel Y axis size" status=0
Record 22: "INSTRUME= 'QHY600M' / Imaging instrument name" status=0
Record 23: "CAMERAID= 'QHY600M-33d3d743814b8b447' / Imaging instrument identifier" status=0
Record 24: "SET-TEMP= -15.0 / [degC] CCD temperature setpoint" status=0
Record 25: "CCD-TEMP= -15.0 / [degC] CCD temperature" status=0
Record 26: "READOUTM= '2CMS-0' / Sensor readout mode" status=0
Record 27: "USBLIMIT= 50 / Camera-specific USB setting" status=0
Record 28: "TELESCOP= 'QHY600M-TTU1' / Name of telescope" status=0
Record 29: "FOCALLEN= 135.0 / [mm] Focal length" status=0
Record 30: "FOCRATIO= 2.2 / Focal ratio" status=0
Record 31: "RA = 323.999919758036 / [deg] RA of telescope" status=0
Record 32: "DEC = 45.9995019204089 / [deg] Declination of telescope" status=0
Record 33: "CENTALT = 33.6991666666667 / [deg] Altitude of telescope" status=0
Record 34: "CENTAZ = 306.608055555556 / [deg] Azimuth of telescope" status=0
Record 35: "AIRMASS = 1.7984810729662 / Airmass at frame center (Gueymard 1993)" status=0
Record 36: "PIERSIDE= 'East' / Telescope pointing state" status=0
Record 37: "SITEELEV= 1013.0 / [m] Observation site elevation" status=0
Record 38: "SITELAT = 33.748239 / [deg] Observation site latitude" status=0
Record 39: "SITELONG= -101.958391 / [deg] Observation site longitude" status=0
Record 40: "OBSERVER= 'Sokolovsky' / Observer name" status=0
Record 41: "OBSERVAT= 'TTU Skyview' / Observatory name" status=0
Record 42: "SITENAME= '' / Observatory site name" status=0
Record 43: "FWHEEL = 'Simulator' / Filter Wheel name" status=0
Record 44: "FILTER = 'CV' / Active filter name" status=0
Record 45: "OBJECT = 'Cyg-04' / Name of the object of interest" status=0
Record 46: "OBJCTRA = '21 36 00' / [H M S] RA of imaged object" status=0
Record 47: "OBJCTDEC= '+46 00 00' / [D M S] Declination of imaged object" status=0
Record 48: "OBJCTROT= 0.0 / [deg] planned rotation of imaged object" status=0
Record 49: "ROWORDER= 'TOP-DOWN' / FITS Image Orientation" status=0
Record 50: "EQUINOX = 2000.0 / Equinox of celestial coordinate system" status=0
Record 51: "SWCREATE= 'N.I.N.A. 3.2.0.9001 (x64)' / Software that created this file" status=0
Record 52: "QHY_EXP = 20.000096 / [s] Actual exposure time" status=0
Record 53: "QHY_PP = 13888.0 / [ps] pixelPeriod" status=0
Record 54: "QHY_LP = 85000.0 / [ns] linePeriod" status=0
Record 55: "GPS_LP = 85000.0 / [ns] linePeriod" status=0
Record 56: "QHY_FP = 20000160.0 / [us] framePeriod" status=0
Record 57: "QHY_CPL = 6120.0 / clocksPerLine" status=0
Record 58: "QHY_LPF = 235295.0 / linesPerFrame" status=0
Record 59: "QHY_AET = 20000096.0 / [us] actualExposureTime" status=0
Record 60: "QHY_LEM = T / isLongExposureMode" status=0
Record 61: "QHY_OFF0= 3767.777 / [us] RollingShutterEndOffset row 0" status=0
Allocating memory for image, dark and result arrays...
Reading image /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits 9576 6388 16 bitpix
SET-TEMP= -15.000000 for /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits
SET-TEMP= -15.000000 for /var/www/nmw_calibration/TTUQ1b1x1/darks/mdark_TTUQ1b1x1_-15C_20s_2026-01-08.fit
CCD-TEMP= -15.000000 for /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits
CCD-TEMP= -15.000000 for /var/www/nmw_calibration/TTUQ1b1x1/darks/mdark_TTUQ1b1x1_-15C_20s_2026-01-08.fit
Reading dark frame /var/www/nmw_calibration/TTUQ1b1x1/darks/mdark_TTUQ1b1x1_-15C_20s_2026-01-08.fit 9576 6388 16 bitpix
Dark frame is subtracted, output is written to /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/d_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits :)
Spent 0.531844 seconds
renamed 'mdark_TTUQ1b1x1_-15C_20s_2026-01-08.png' -> 'transient_report/dark.png'
MegaDivider v7
Reading image /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/d_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits 9576 6388 16 bitpix
Reading flat /var/www/nmw_calibration/TTUQ1b1x1/flats/mff_TTUQ1b1x1_2025-12-22.fit 9576 6388 16 bitpix
Avarage count on flat field image: 38918.354428
Minimal real count (from overscan): 5
Output is written to /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits :)
No overscan detected - all values seem high! (left_median=27736.5, right_median=26453.5)
renamed 'mff_TTUQ1b1x1_2025-12-22.png' -> 'transient_report/flat.png'
Using calibrated image CALIBRATED_SECOND_EPOCH__SECOND_IMAGE=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits
Dark frame used to calibrate the second-epoch images:
Flat field used to calibrate the second-epoch images:
after the calibration attempt:
SECOND_EPOCH__FIRST_IMAGE=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits
SECOND_EPOCH__SECOND_IMAGE=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits
Previews of the CALIBRATED second-epoch images:
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461061.55555686
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits exists and is non-empty
Saving wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits to local_wcs_cache/
'wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits' -> 'local_wcs_cache/wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits'
wcs_Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits exists and is non-empty
Saving wcs_Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits to local_wcs_cache/
'wcs_Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits' -> 'local_wcs_cache/wcs_Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits'
wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits exists and is non-empty
Saving wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits to local_wcs_cache/
'wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits' -> 'local_wcs_cache/wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits'
wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits exists and is non-empty
Saving wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits to local_wcs_cache/
'wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits' -> 'local_wcs_cache/wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 21:35:56.988 +45:59:46.04
Second-epoch image center 21:36:05.104 +45:59:44.71
Angular distance between the image centers 0.02 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 21:35:56.988 +45:59:46.04
Second-epoch image center 21:36:07.919 +46:00:44.76
Angular distance between the image centers 0.04 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 21:36:05.104 +45:59:44.71
Second-epoch second image center 21:36:07.919 +46:00:44.76
Angular distance between the image centers 0.01856 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits &> /tmp/tmp.wWt7wATHvE
Parallel run for /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits &> /tmp/tmp.VEHTCONUes
Parallel run for /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits &> /tmp/tmp.GxcXbYycSc
Parallel run for /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits &> /tmp/tmp.P9fy7wUZRM
Parallel run for /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits and wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits and wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits.cat
Found non-empty wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits and wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits.cat
The reference image (wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits) and catalog (wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits.cat) found
'wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits.cat' -> 'wcsmag.cat'
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 3826 out of 34779 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.925460
a=0.000000 b=1.000000 c=22.925460
From vast_summary.log: estimated ref. image limiting mag.: -7.90
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.03
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.03
____ End of magnitude calibration ____
Filter-out faint candidates...
Filter-out suspiciously bright candidates...
Filter-out candidates with large difference between measured mags in one epoch...
Filter-out small-amplitude flares...
Preparing the exclusion lists for this field
Done with filtering
Found 50 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits
2.2 pix Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits
2.1 pix fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits
2.1 pix fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits
Limiting magnitude estimates:
15.0 mag. Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits
15.0 mag. Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits
14.9 mag. fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits
14.9 mag. fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits
All-image limiting magnitude estimate: 14.9 (SNR ) 12.0 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.wWt7wATHvE (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate...
/mnt/usb2/NMW-TexasTech/workdir/vast_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/util/wcs_image_calibration.sh /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits
FITSFILE before on_the_fly=/mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits
FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits
verification OK: /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits has a WCS header - will blindly trust it is good...
'/mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits' -> 'wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits'
FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits
WCS_IMAGE_NAME=wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits
WCS-calibrated image found: wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits
Checking if the catalog wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits.cat corresponding to the image wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits alredy exist and is non-empty...
Catalog wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits.cat corresponding to the image wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits
WCS catalog name: wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits.cat
The fraction of blended stars is high!
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=4546, passed=34779
Got 34779 stars (including 30191 good ones) from the SExtractor catalog wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits.cat
util/solve_plate_with_UCAC5 got 34779 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 584 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 4.40"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 3.76"
ITERATION 02 -- talking to VizieR, this might be slow!
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 642 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 3.73"
Estimated accuracy of the plate solution: 2.56"
Excluding outliers - 578 stars left (next iteration limit 559)
The image catalog is written to wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits.cat.ds9.reg
You may view it with the command:
ds9 /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits -region wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.VEHTCONUes (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate...
/mnt/usb2/NMW-TexasTech/workdir/vast_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/util/wcs_image_calibration.sh /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits
FITSFILE before on_the_fly=/mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits
FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits
verification OK: /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits has a WCS header - will blindly trust it is good...
'/mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits' -> 'wcs_Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits'
FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits
WCS_IMAGE_NAME=wcs_Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits
WCS-calibrated image found: wcs_Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits
Checking if the catalog wcs_Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits.cat corresponding to the image wcs_Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits alredy exist and is non-empty...
Catalog wcs_Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits.cat corresponding to the image wcs_Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits
WCS catalog name: wcs_Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits.cat
The fraction of blended stars is high!
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=4537, passed=34638
Got 34638 stars (including 30059 good ones) from the SExtractor catalog wcs_Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits.cat
util/solve_plate_with_UCAC5 got 34638 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010466 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 709 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 2.14"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 2.63"
ITERATION 02 -- talking to VizieR, this might be slow!
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 765 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 2.61"
Estimated accuracy of the plate solution: 1.65"
Excluding outliers - 731 stars left (next iteration limit 726)
The image catalog is written to wcs_Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits.cat.ds9.reg
You may view it with the command:
ds9 /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits -region wcs_Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.GxcXbYycSc (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate...
/mnt/usb2/NMW-TexasTech/workdir/vast_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/util/wcs_image_calibration.sh /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits
FITSFILE before on_the_fly=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits
FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits
verification OK: /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits
WCS-calibrated image found: wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits
Checking if the catalog wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits.cat corresponding to the image wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits.cat corresponding to the image wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits
WCS catalog name: wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits.cat
The fraction of blended stars is high!
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3368, passed=31029
Got 31029 stars (including 27613 good ones) from the SExtractor catalog wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits.cat
util/solve_plate_with_UCAC5 got 31029 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.1'
Seting catalog search parameters based on the expected field of view 942.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013085 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010468 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 789 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 5.39"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 4.63"
ITERATION 02 -- talking to VizieR, this might be slow!
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 784 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 4.55"
Estimated accuracy of the plate solution: 2.79"
Excluding outliers - 751 stars left (next iteration limit 775)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits.cat.ds9.reg
You may view it with the command:
ds9 /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits -region wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.P9fy7wUZRM (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate...
/mnt/usb2/NMW-TexasTech/workdir/vast_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/util/wcs_image_calibration.sh /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits
FITSFILE before on_the_fly=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits
FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits
verification OK: /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits
WCS-calibrated image found: wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits
Checking if the catalog wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits.cat corresponding to the image wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits.cat corresponding to the image wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits
WCS catalog name: wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits.cat
The fraction of blended stars is high!
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3502, passed=30919
Got 30919 stars (including 27379 good ones) from the SExtractor catalog wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits.cat
util/solve_plate_with_UCAC5 got 30919 stars from the SExtractor catalog
/mnt/usb2/NMW-TexasTech/workdir/vast_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 637 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 3.12"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 2.99"
ITERATION 02 -- talking to VizieR, this might be slow!
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 680 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 2.96"
Estimated accuracy of the plate solution: 1.80"
Excluding outliers - 636 stars left (next iteration limit 645)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits.cat.ds9.reg
You may view it with the command:
ds9 /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits -region wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits' -> '/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits'
Saving fully-calibrated image wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits' -> '/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits'
Preparing the HTML report for the field Cyg-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Adding exclusion_list_local.txt__out52430.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52432.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52433.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52448.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52450.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52451.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52456.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52457.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52458.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52462.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52464.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52480.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52481.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52484.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52485.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52486.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52498.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52512.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52517.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52538.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52542.dat to exclusion_list_local.txt
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52422_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 52422_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (15.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52430_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 52430_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/52430_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/52430_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/52430_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52432_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 52432_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/52432_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/52432_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/52432_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52433_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 52433_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/52433_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/52433_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/52433_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52434_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 52434_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (311.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52436_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 52436_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (248.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52447_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 52447_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (425.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52448_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 52448_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/52448_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/52448_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/52448_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52449_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 52449_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 21:42:00.46 +45:47:30.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52450_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 52450_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/52450_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/52450_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/52450_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52451_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 52451_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/52451_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/52451_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/52451_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52452_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 52452_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (48.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52454_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 52454_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (649.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52455_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 52455_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52456_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 52456_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/52456_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/52456_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/52456_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52457_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 52457_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/52457_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/52457_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/52457_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52458_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 52458_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/52458_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/52458_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/52458_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52462_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 52462_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/52462_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/52462_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/52462_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52464_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 52464_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/52464_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/52464_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/52464_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52465_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 52465_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (53.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52466_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 52466_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (420.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52469_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 52469_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (15.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52472_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 52472_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52473_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 52473_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (14.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52478_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 52478_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52480_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 52480_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/52480_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/52480_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/52480_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52481_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 52481_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/52481_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/52481_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/52481_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52484_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 52484_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/52484_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/52484_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/52484_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52485_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 52485_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/52485_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/52485_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/52485_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52486_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 52486_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/52486_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/52486_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/52486_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52487_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 52487_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (193.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52492_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 52492_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (266.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52493_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 52493_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52494_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 52494_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (64.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52497_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 52497_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (60.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52498_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 52498_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/52498_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/52498_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/52498_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52499_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 52499_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52511_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 52511_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52512_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 52512_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/52512_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/52512_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/52512_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52516_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 52516_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (16.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52517_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 52517_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/52517_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/52517_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/52517_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52523_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 52523_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52524_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 52524_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (673.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52529_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 52529_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (107.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52532_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 52532_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (28.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52538_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 52538_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/52538_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/52538_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/52538_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52540_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 52540_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (762.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52542_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 52542_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/52542_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/52542_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/52542_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07403_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 07403_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 21:52:52.37 +48:57:24.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34131_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 34131_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (782.3") between the two second-epoch detections
Prepared the HTML report for the field Cyg-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
22:09:24.00 +47:56:36.1
21:22:33.84 +48:57:03.7
22:19:28.00 +50:11:11.7
21:31:22.14 +48:26:44.0
22:03:43.48 +49:45:23.7
22:08:59.96 +48:32:00.5
21:38:00.57 +48:28:18.6
21:36:35.43 +47:32:50.0
21:29:03.93 +51:14:20.1
21:57:08.84 +49:52:16.7
22:10:58.49 +46:27:24.1
21:29:40.60 +49:49:53.6
22:16:36.54 +49:26:23.5
21:28:03.62 +49:15:08.4
21:38:02.80 +49:24:22.3
21:37:42.38 +47:26:32.9
22:04:34.59 +49:35:30.8
21:16:46.25 +44:55:20.8
21:18:09.66 +48:55:21.5
21:34:36.84 +47:42:37.2
21:31:01.06 +47:48:28.3
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits
Creating symlink local_wcs_cache/wcs_Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits
Creating symlink local_wcs_cache/wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits
Creating symlink local_wcs_cache/wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Creating symlink local_wcs_cache/exclusion_list_bbsc.txt
Creating symlink local_wcs_cache/exclusion_list_bsc.txt
Creating symlink local_wcs_cache/exclusion_list_tycho2.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits exists and is non-empty
wcs_Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits exists and is non-empty
wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits exists and is non-empty
wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 21:35:56.988 +45:59:46.04
Second-epoch image center 21:36:05.104 +45:59:44.71
Angular distance between the image centers 0.02 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 21:35:56.988 +45:59:46.04
Second-epoch image center 21:36:07.919 +46:00:44.76
Angular distance between the image centers 0.04 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 21:36:05.104 +45:59:44.71
Second-epoch second image center 21:36:07.919 +46:00:44.76
Angular distance between the image centers 0.01856 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits &> /tmp/tmp.05KeMphzuk
Parallel run for /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits &> /tmp/tmp.vyxlcVih8C
Parallel run for /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits &> /tmp/tmp.boqjiTWWcI
Parallel run for /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits &> /tmp/tmp.6KYvmhh1kG
Parallel run for /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits and wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits and wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits.cat
Found non-empty wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits and wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits.cat
The reference image (wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits) and catalog (wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits.cat) found
'wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits.cat' -> 'wcsmag.cat'
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 4088 out of 260598 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.697265
a=0.000000 b=1.000000 c=22.697265
From vast_summary.log: estimated ref. image limiting mag.: -7.57
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.13
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.13
____ End of magnitude calibration ____
Filter-out faint candidates...
Filter-out suspiciously bright candidates...
Filter-out candidates with large difference between measured mags in one epoch...
Filter-out small-amplitude flares...
Preparing the exclusion lists for this field
Done with filtering
Found 1274 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits
2.0 pix Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits
2.0 pix fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits
1.9 pix fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits
Limiting magnitude estimates:
15.1 mag. Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits
15.1 mag. Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits
15.0 mag. fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits
15.0 mag. fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 14.3 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.05KeMphzuk (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate...
/mnt/usb2/NMW-TexasTech/workdir/vast_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/util/wcs_image_calibration.sh /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits
FITSFILE before on_the_fly=/mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits
FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits
verification OK: /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits has a WCS header - will blindly trust it is good...
'/mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits' -> 'wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits'
FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits
WCS_IMAGE_NAME=wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits
WCS-calibrated image found: wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits
Checking if the catalog wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits.cat corresponding to the image wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits alredy exist and is non-empty...
Catalog wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits.cat corresponding to the image wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits
WCS catalog name: wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits.cat
The fraction of blended stars is high!
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=49, blended=52643, passed=260549
Got 260549 stars (including 207583 good ones) from the SExtractor catalog wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits.cat
util/solve_plate_with_UCAC5 got 260549 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 576 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 4.52"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 3.87"
ITERATION 02 -- talking to VizieR, this might be slow!
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 636 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 3.87"
Estimated accuracy of the plate solution: 2.37"
Excluding outliers - 577 stars left (next iteration limit 557)
The image catalog is written to wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits.cat.ds9.reg
You may view it with the command:
ds9 /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits -region wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.vyxlcVih8C (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate...
/mnt/usb2/NMW-TexasTech/workdir/vast_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/util/wcs_image_calibration.sh /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits
FITSFILE before on_the_fly=/mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits
FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits
verification OK: /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits has a WCS header - will blindly trust it is good...
'/mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits' -> 'wcs_Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits'
FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits
WCS_IMAGE_NAME=wcs_Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits
WCS-calibrated image found: wcs_Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits
Checking if the catalog wcs_Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits.cat corresponding to the image wcs_Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits alredy exist and is non-empty...
Catalog wcs_Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits.cat corresponding to the image wcs_Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits
WCS catalog name: wcs_Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits.cat
The fraction of blended stars is high!
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=61, blended=53402, passed=262622
Got 262622 stars (including 208887 good ones) from the SExtractor catalog wcs_Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits.cat
util/solve_plate_with_UCAC5 got 262622 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010466 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 701 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 1.99"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 2.19"
ITERATION 02 -- talking to VizieR, this might be slow!
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 746 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 2.18"
Estimated accuracy of the plate solution: 1.57"
Excluding outliers - 721 stars left (next iteration limit 731)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits.cat.ds9.reg
You may view it with the command:
ds9 /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits -region wcs_Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.boqjiTWWcI (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate...
/mnt/usb2/NMW-TexasTech/workdir/vast_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/util/wcs_image_calibration.sh /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits
FITSFILE before on_the_fly=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits
FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits
verification OK: /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits
WCS-calibrated image found: wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits
Checking if the catalog wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits.cat corresponding to the image wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits.cat corresponding to the image wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits
WCS catalog name: wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits.cat
The fraction of blended stars is high!
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=31, blended=41315, passed=240613
Got 240613 stars (including 199035 good ones) from the SExtractor catalog wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits.cat
util/solve_plate_with_UCAC5 got 240613 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.1'
Seting catalog search parameters based on the expected field of view 942.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013085 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010468 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 784 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 4.81"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 4.46"
ITERATION 02 -- talking to VizieR, this might be slow!
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 791 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 4.46"
Estimated accuracy of the plate solution: 2.43"
Excluding outliers - 759 stars left (next iteration limit 779)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits.cat.ds9.reg
You may view it with the command:
ds9 /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits -region wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.6KYvmhh1kG (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate...
/mnt/usb2/NMW-TexasTech/workdir/vast_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/util/wcs_image_calibration.sh /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits
FITSFILE before on_the_fly=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits
FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits
verification OK: /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits
WCS-calibrated image found: wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits
Checking if the catalog wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits.cat corresponding to the image wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits.cat corresponding to the image wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits
WCS catalog name: wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits.cat
The fraction of blended stars is high!
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=43, blended=43005, passed=247349
Got 247349 stars (including 204043 good ones) from the SExtractor catalog wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits.cat
util/solve_plate_with_UCAC5 got 247349 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 636 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 2.89"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 3.04"
ITERATION 02 -- talking to VizieR, this might be slow!
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 664 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 3.04"
Estimated accuracy of the plate solution: 1.70"
Excluding outliers - 619 stars left (next iteration limit 636)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits.cat.ds9.reg
You may view it with the command:
ds9 /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits -region wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.fits
Saving fully-calibrated image wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-04-Q1b1x1_205845_TTUQ1b1x1_5338_kW8Yhzdp/wcs_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.fits
Preparing the HTML report for the field Cyg-04-Q1b1x1 with default.sex.telephoto_lens_vSTL
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Adding exclusion_list_gaiadr2.txt__out296792.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296797.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296816.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296858.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296867.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296870.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296872.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296887.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296910.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296920.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296991.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out297016.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out297018.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out297023.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out297031.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out297074.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out297082.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out297111.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out297178.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out297181.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out297263.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out297302.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out297351.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out297548.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out297693.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out297892.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out298126.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out298314.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out298553.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out298684.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out298745.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out298803.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out296413.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296519.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296539.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296591.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296630.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296631.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296632.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296636.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296651.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296669.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296699.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296700.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296783.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296786.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296811.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296840.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296841.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296864.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296866.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296871.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296879.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296880.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296885.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296907.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296919.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296930.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296947.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296951.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296955.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296962.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296999.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297024.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297028.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297039.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297040.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297041.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297047.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297050.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297052.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297056.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297058.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297059.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297065.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297066.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297072.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297077.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297085.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297101.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297105.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297108.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297109.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297112.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297118.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297119.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297122.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297123.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297127.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297128.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297131.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297133.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297139.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297144.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297146.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297148.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297155.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297156.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297157.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297160.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297161.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297166.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297171.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297172.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297174.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297176.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297184.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297185.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297186.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297190.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297192.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297199.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297201.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297202.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297209.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297212.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297213.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297214.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297217.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297220.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297222.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297225.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297226.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297230.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297235.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297236.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297238.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297240.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297242.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297243.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297248.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297249.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297251.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297252.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297255.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297261.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297262.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297267.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297268.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297269.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297273.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297278.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297279.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297285.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297287.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297288.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297290.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297291.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297294.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297310.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297317.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297318.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297326.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297327.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297329.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297332.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297335.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297341.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297342.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297348.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297349.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297353.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297354.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297363.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297366.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297368.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297370.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297376.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297383.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297392.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297394.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297396.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297399.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297403.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297404.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297407.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297408.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297413.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297420.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297421.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297422.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297423.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297425.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297436.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297438.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297439.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297443.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297453.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297455.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297462.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297468.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297469.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297473.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297474.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297475.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297476.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297481.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297484.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297490.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297496.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297501.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297505.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297511.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297514.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297517.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297520.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297533.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297536.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297538.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297539.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297540.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297541.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297568.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297573.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297592.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297610.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297611.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297616.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297620.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297627.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297634.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297639.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297643.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297645.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297653.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297661.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297684.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297686.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297708.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297709.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297711.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297717.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297743.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297750.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297752.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297766.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297778.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297790.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297792.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297794.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297800.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297802.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297806.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297814.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297829.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297837.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297869.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297875.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297894.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297899.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297903.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297914.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297916.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297920.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297923.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297951.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297974.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297992.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297993.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297996.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297999.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out298009.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out298030.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out298047.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out298084.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out298091.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out298110.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out298116.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out298117.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out298125.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out298131.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out298137.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out298139.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out298142.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out298159.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out298160.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out298164.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out298182.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out298245.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out298247.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out298251.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out298258.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out298278.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out298289.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out298310.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out298326.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out298335.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out298336.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out298364.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out298370.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out298376.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out298383.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out298406.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out298410.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out298412.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out298414.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out298452.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out298489.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out298514.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out298539.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out298544.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out298547.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out298554.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out298565.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out298573.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out298598.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out298659.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out298682.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out298702.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out298717.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out298718.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out298740.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out298928.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out298942.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out299035.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35454.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37316.dat to exclusion_list_local.txt
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296291_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296291_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (222.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296342_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296342_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296358_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296358_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296378_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296378_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296380_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296380_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (720.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296381_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296381_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296389_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296389_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (273.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296391_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296391_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296408_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296408_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296413_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 296413_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/296413_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/296413_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/296413_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296416_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296416_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296417_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296417_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (557.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296418_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296418_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296421_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296421_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (104.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296423_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296423_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296427_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296427_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (16.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296429_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296429_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (39.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296430_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296430_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296440_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296440_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296441_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296441_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (16.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296448_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296448_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296453_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296453_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (13.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296463_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296463_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296469_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296469_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296470_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296470_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296473_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296473_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (46.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296475_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296475_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (86.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296481_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296481_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296483_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296483_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296486_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296486_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296489_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296489_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296492_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296492_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (463.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296496_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296496_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296498_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296498_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296499_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296499_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (16.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296504_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296504_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296512_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296512_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296515_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296515_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (23.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296516_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296516_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296517_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296517_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296519_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 296519_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/296519_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/296519_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/296519_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296522_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296522_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296523_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296523_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296524_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296524_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296525_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296525_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296527_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296527_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296528_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296528_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296529_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296529_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296530_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296530_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (283.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296531_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296531_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296536_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296536_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296537_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296537_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (653.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296539_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 296539_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/296539_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/296539_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/296539_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296541_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296541_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (18.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296543_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296543_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (634.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296548_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296548_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296553_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296553_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296555_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296555_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296556_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296556_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (17.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296560_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296560_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296561_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296561_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (34.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296564_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296564_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (24.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296570_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296570_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296574_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296574_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296577_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296577_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296585_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296585_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296586_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296586_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (318.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296591_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 296591_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/296591_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/296591_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/296591_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296592_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296592_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296594_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296594_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (18.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296596_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296596_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296598_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296598_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (16.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296599_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296599_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296600_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296600_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296601_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296601_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (188.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296605_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296605_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296611_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296611_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296613_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296613_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (884.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296616_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296616_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (306.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296618_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296618_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (16.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296622_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296622_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296625_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296625_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (15.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296627_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296627_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296628_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296628_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296630_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 296630_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/296630_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/296630_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/296630_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296631_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 296631_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/296631_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/296631_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/296631_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296632_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 296632_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/296632_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/296632_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/296632_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296634_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296634_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (198.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296635_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296635_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296636_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 296636_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/296636_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/296636_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/296636_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296637_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296637_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296642_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296642_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296643_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296643_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296644_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296644_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296645_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296645_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296647_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296647_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296649_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296649_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296651_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 296651_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/296651_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/296651_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/296651_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296659_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296659_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (330.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296660_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296660_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296666_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296666_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (62.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296668_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296668_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296669_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 296669_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/296669_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/296669_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/296669_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296674_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296674_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (363.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296676_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296676_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (401.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296682_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296682_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (292.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296683_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296683_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296685_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296685_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296687_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296687_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296688_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296688_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296689_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296689_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (99.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296690_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296690_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296691_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296691_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296698_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296698_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (624.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296699_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 296699_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/296699_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/296699_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/296699_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296700_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 296700_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/296700_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/296700_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/296700_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296701_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296701_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296702_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296702_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296707_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296707_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296708_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296708_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296710_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296710_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296712_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296712_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296713_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296713_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296715_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296715_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296716_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296716_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296723_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296723_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (330.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296725_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296725_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296729_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296729_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (180.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296731_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296731_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (434.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296733_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296733_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296734_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296734_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (233.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296735_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296735_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (17.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296737_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296737_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296739_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296739_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296742_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296742_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296745_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296745_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296746_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296746_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (17.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296747_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296747_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (339.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296749_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296749_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (13.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296753_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296753_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296757_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296757_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (553.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296759_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296759_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (46.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296765_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296765_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296768_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296768_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296769_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296769_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (24.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296771_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296771_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296773_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296773_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (429.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296777_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296777_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296778_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296778_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (323.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296779_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296779_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296780_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296780_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296783_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 296783_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/296783_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/296783_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/296783_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296786_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 296786_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/296786_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/296786_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/296786_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296790_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296790_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296791_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296791_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296792_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296792_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 21:59:21.51 +48:33:18.7 in Gaia DR2 blend (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.98, BLEND_MAG_FAINT_SEARCH_LIMIT=, VIZIER_COMMAND=#lib/vizquery -site=vizier.china-vo.org -mime=text -source=I/345/gaia2 -out.max=3 -out.add=_r -out.form=mini -sort=Gmag Gmag=0.0..14.96 -c=21:59:21.51 +48:33:18.7 -c.rs=14.75 -out=Source,RA_ICRS,DE_ICRS,Gmag,RPmag,Var#)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296793_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296793_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (224.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296795_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296795_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (16.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296797_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296797_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 21:57:59.76 +48:41:28.0 in Gaia DR2 blend (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.01, BLEND_MAG_FAINT_SEARCH_LIMIT=, VIZIER_COMMAND=#lib/vizquery -site=vizier.china-vo.org -mime=text -source=I/345/gaia2 -out.max=3 -out.add=_r -out.form=mini -sort=Gmag Gmag=0.0..14.99 -c=21:57:59.76 +48:41:28.0 -c.rs=14.75 -out=Source,RA_ICRS,DE_ICRS,Gmag,RPmag,Var#)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296798_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296798_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296801_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296801_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (14.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296802_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296802_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (788.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296804_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296804_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (16.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296807_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296807_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (32.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296811_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 296811_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/296811_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/296811_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/296811_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296812_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296812_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (380.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296814_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296814_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296816_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296816_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 22:01:53.19 +47:44:17.9 in Gaia DR2 blend (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.05, BLEND_MAG_FAINT_SEARCH_LIMIT=, VIZIER_COMMAND=#lib/vizquery -site=vizier.china-vo.org -mime=text -source=I/345/gaia2 -out.max=3 -out.add=_r -out.form=mini -sort=Gmag Gmag=0.0..15.03 -c=22:01:53.19 +47:44:17.9 -c.rs=14.75 -out=Source,RA_ICRS,DE_ICRS,Gmag,RPmag,Var#)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296820_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296820_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (165.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296822_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296822_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296824_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296824_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296825_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296825_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (398.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296830_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296830_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296838_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296838_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296839_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296839_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296840_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 296840_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/296840_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/296840_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/296840_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296841_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 296841_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/296841_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/296841_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/296841_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296842_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296842_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (51.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296848_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296848_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296849_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296849_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296850_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296850_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296851_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296851_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296855_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296855_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (167.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296857_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296857_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (857.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296858_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296858_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 21:58:54.54 +48:40:20.6 in Gaia DR2 blend (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.85, BLEND_MAG_FAINT_SEARCH_LIMIT=, VIZIER_COMMAND=#lib/vizquery -site=vizier.china-vo.org -mime=text -source=I/345/gaia2 -out.max=3 -out.add=_r -out.form=mini -sort=Gmag Gmag=0.0..14.83 -c=21:58:54.54 +48:40:20.6 -c.rs=14.75 -out=Source,RA_ICRS,DE_ICRS,Gmag,RPmag,Var#)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296859_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296859_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296864_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 296864_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/296864_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/296864_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/296864_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296865_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296865_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296866_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 296866_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/296866_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/296866_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/296866_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296867_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296867_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 22:00:29.95 +48:38:29.7 in Gaia DR2 blend (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.94, BLEND_MAG_FAINT_SEARCH_LIMIT=, VIZIER_COMMAND=#lib/vizquery -site=vizier.china-vo.org -mime=text -source=I/345/gaia2 -out.max=3 -out.add=_r -out.form=mini -sort=Gmag Gmag=0.0..14.92 -c=22:00:29.95 +48:38:29.7 -c.rs=14.75 -out=Source,RA_ICRS,DE_ICRS,Gmag,RPmag,Var#)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296868_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296868_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296870_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296870_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 22:15:51.27 +48:55:60.0 in Gaia DR2 single (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80, VIZIER_COMMAND=#lib/vizquery -site=vizier.china-vo.org -mime=text -source=I/345/gaia2 -out.max=3 -out.add=_r -out.form=mini -sort=Gmag Gmag=0.0..14.80 -c=22:15:51.27 +48:55:60.0 -c.rs=14.75 -out=Source,RA_ICRS,DE_ICRS,Gmag,RPmag,Var#)VIZIER_GAIADR2_OUTPUT=# 2.865 1999691452524673792 333.96469253377 +48.93370960496 12.6003 11.7264 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.865#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296871_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 296871_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/296871_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/296871_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/296871_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296872_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296872_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 21:58:48.78 +48:43:25.1 in Gaia DR2 blend (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.81, BLEND_MAG_FAINT_SEARCH_LIMIT=, VIZIER_COMMAND=#lib/vizquery -site=vizier.china-vo.org -mime=text -source=I/345/gaia2 -out.max=3 -out.add=_r -out.form=mini -sort=Gmag Gmag=0.0..14.79 -c=21:58:48.78 +48:43:25.1 -c.rs=14.75 -out=Source,RA_ICRS,DE_ICRS,Gmag,RPmag,Var#)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296873_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296873_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296876_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296876_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296878_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296878_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296879_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 296879_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/296879_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/296879_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/296879_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296880_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 296880_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/296880_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/296880_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/296880_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296881_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296881_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296885_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 296885_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/296885_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/296885_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/296885_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296886_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296886_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296887_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296887_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 21:52:38.04 +49:47:56.3 in Gaia DR2 blend (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.84, BLEND_MAG_FAINT_SEARCH_LIMIT=, VIZIER_COMMAND=#lib/vizquery -site=vizier.china-vo.org -mime=text -source=I/345/gaia2 -out.max=3 -out.add=_r -out.form=mini -sort=Gmag Gmag=0.0..14.82 -c=21:52:38.04 +49:47:56.3 -c.rs=14.75 -out=Source,RA_ICRS,DE_ICRS,Gmag,RPmag,Var#)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296889_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296889_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296895_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296895_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296897_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296897_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (14.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296903_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296903_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (711.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296907_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 296907_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/296907_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/296907_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/296907_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296910_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296910_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 22:12:51.01 +48:30:45.0 in Gaia DR2 blend (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.79, BLEND_MAG_FAINT_SEARCH_LIMIT=, VIZIER_COMMAND=#lib/vizquery -site=vizier.china-vo.org -mime=text -source=I/345/gaia2 -out.max=3 -out.add=_r -out.form=mini -sort=Gmag Gmag=0.0..14.77 -c=22:12:51.01 +48:30:45.0 -c.rs=14.75 -out=Source,RA_ICRS,DE_ICRS,Gmag,RPmag,Var#)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296912_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296912_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296917_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296917_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (16.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296918_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296918_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296919_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 296919_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/296919_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/296919_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/296919_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296920_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296920_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 21:39:41.79 +50:21:50.1 in Gaia DR2 blend (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.87, BLEND_MAG_FAINT_SEARCH_LIMIT=, VIZIER_COMMAND=#lib/vizquery -site=vizier.china-vo.org -mime=text -source=I/345/gaia2 -out.max=3 -out.add=_r -out.form=mini -sort=Gmag Gmag=0.0..14.85 -c=21:39:41.79 +50:21:50.1 -c.rs=14.75 -out=Source,RA_ICRS,DE_ICRS,Gmag,RPmag,Var#)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296922_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296922_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (474.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296925_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296925_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296926_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296926_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (14.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296927_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296927_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296930_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 296930_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/296930_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/296930_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/296930_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296931_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296931_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (32.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296932_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296932_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296936_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296936_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (776.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296942_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296942_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296943_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296943_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (64.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296946_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296946_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296947_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 296947_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/296947_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/296947_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/296947_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296949_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296949_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296950_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296950_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (34.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296951_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 296951_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/296951_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/296951_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/296951_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296954_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296954_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (151.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296955_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 296955_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/296955_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/296955_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/296955_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296957_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296957_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296960_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296960_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (306.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296961_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296961_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (797.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296962_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 296962_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/296962_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/296962_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/296962_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296963_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296963_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296964_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296964_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (196.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296968_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296968_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (31.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296970_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296970_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (52.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296971_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296971_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (13.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296972_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296972_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296974_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296974_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296975_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296975_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (720.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296977_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296977_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296978_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296978_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296979_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296979_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296980_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296980_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296981_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296981_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296985_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296985_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296988_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296988_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (61.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296990_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296990_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296991_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296991_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 22:00:27.14 +48:17:42.6 in Gaia DR2 blend (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.39, BLEND_MAG_FAINT_SEARCH_LIMIT=, VIZIER_COMMAND=#lib/vizquery -site=vizier.china-vo.org -mime=text -source=I/345/gaia2 -out.max=3 -out.add=_r -out.form=mini -sort=Gmag Gmag=0.0..14.37 -c=22:00:27.14 +48:17:42.6 -c.rs=14.75 -out=Source,RA_ICRS,DE_ICRS,Gmag,RPmag,Var#)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296992_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296992_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296994_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296994_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296996_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 296996_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296999_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 296999_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/296999_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/296999_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/296999_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297000_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297000_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (93.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297001_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297001_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297004_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297004_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297005_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297005_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (87.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297009_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297009_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (862.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297011_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297011_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297013_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297013_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297014_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297014_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297015_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297015_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297016_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297016_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 22:16:01.22 +49:43:05.5 in Gaia DR2 blend (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.29, BLEND_MAG_FAINT_SEARCH_LIMIT=, VIZIER_COMMAND=#lib/vizquery -site=vizier.china-vo.org -mime=text -source=I/345/gaia2 -out.max=3 -out.add=_r -out.form=mini -sort=Gmag Gmag=0.0..14.27 -c=22:16:01.22 +49:43:05.5 -c.rs=14.75 -out=Source,RA_ICRS,DE_ICRS,Gmag,RPmag,Var#)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297018_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297018_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 21:59:57.24 +48:35:44.0 in Gaia DR2 blend (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.17, BLEND_MAG_FAINT_SEARCH_LIMIT=, VIZIER_COMMAND=#lib/vizquery -site=vizier.china-vo.org -mime=text -source=I/345/gaia2 -out.max=3 -out.add=_r -out.form=mini -sort=Gmag Gmag=0.0..14.15 -c=21:59:57.24 +48:35:44.0 -c.rs=14.75 -out=Source,RA_ICRS,DE_ICRS,Gmag,RPmag,Var#)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297019_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297019_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297022_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297022_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297023_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297023_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 22:16:08.33 +47:44:52.4 in Gaia DR2 blend (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.37, BLEND_MAG_FAINT_SEARCH_LIMIT=, VIZIER_COMMAND=#lib/vizquery -site=vizier.china-vo.org -mime=text -source=I/345/gaia2 -out.max=3 -out.add=_r -out.form=mini -sort=Gmag Gmag=0.0..14.35 -c=22:16:08.33 +47:44:52.4 -c.rs=14.75 -out=Source,RA_ICRS,DE_ICRS,Gmag,RPmag,Var#)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297024_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297024_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297024_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297024_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297024_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297028_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297028_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297028_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297028_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297028_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297031_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297031_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 22:06:11.46 +49:35:37.8 in Gaia DR2 blend (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.19, BLEND_MAG_FAINT_SEARCH_LIMIT=, VIZIER_COMMAND=#lib/vizquery -site=vizier.china-vo.org -mime=text -source=I/345/gaia2 -out.max=3 -out.add=_r -out.form=mini -sort=Gmag Gmag=0.0..14.17 -c=22:06:11.46 +49:35:37.8 -c.rs=14.75 -out=Source,RA_ICRS,DE_ICRS,Gmag,RPmag,Var#)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297032_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297032_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (16.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297033_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297033_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297035_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297035_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297037_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297037_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (52.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297038_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297038_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297039_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297039_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297039_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297039_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297039_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297040_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297040_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297040_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297040_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297040_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297041_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297041_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297041_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297041_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297041_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297046_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297046_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297047_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297047_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297047_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297047_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297047_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297050_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297050_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297050_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297050_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297050_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297052_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297052_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297052_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297052_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297052_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297055_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297055_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (18.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297056_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297056_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297056_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297056_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297056_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297057_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297057_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (17.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297058_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297058_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297058_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297058_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297058_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297059_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297059_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297059_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297059_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297059_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297060_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297060_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297062_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297062_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297065_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297065_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297065_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297065_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297065_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297066_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297066_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297066_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297066_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297066_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297069_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297069_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297072_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297072_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297072_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297072_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297072_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297074_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297074_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 21:28:05.12 +46:53:01.1 in Gaia DR2 blend (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.27, BLEND_MAG_FAINT_SEARCH_LIMIT=, VIZIER_COMMAND=#lib/vizquery -site=vizier.china-vo.org -mime=text -source=I/345/gaia2 -out.max=3 -out.add=_r -out.form=mini -sort=Gmag Gmag=0.0..13.25 -c=21:28:05.12 +46:53:01.1 -c.rs=14.75 -out=Source,RA_ICRS,DE_ICRS,Gmag,RPmag,Var#)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297077_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297077_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297077_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297077_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297077_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297080_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297080_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297082_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297082_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 21:33:43.11 +50:15:29.5 in Gaia DR2 blend (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=11.98, BLEND_MAG_FAINT_SEARCH_LIMIT=, VIZIER_COMMAND=#lib/vizquery -site=vizier.china-vo.org -mime=text -source=I/345/gaia2 -out.max=3 -out.add=_r -out.form=mini -sort=Gmag Gmag=0.0..12.96 -c=21:33:43.11 +50:15:29.5 -c.rs=14.75 -out=Source,RA_ICRS,DE_ICRS,Gmag,RPmag,Var#)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297085_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297085_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297085_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297085_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297085_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297086_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297086_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (699.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297090_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297090_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (230.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297094_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297094_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 21:50:38.22 +49:25:46.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297097_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297097_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (430.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297098_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297098_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 21:56:13.18 +47:28:30.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297101_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297101_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297101_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297101_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297101_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297102_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297102_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 22:08:59.91 +48:32:01.2 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297103_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297103_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 22:03:43.26 +49:45:24.4 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297105_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297105_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297105_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297105_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297105_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297107_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297107_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 21:33:12.66 +45:49:57.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297108_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297108_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297108_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297108_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297108_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297109_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297109_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297109_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297109_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297109_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297110_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297110_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 21:38:00.28 +48:28:19.3 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297111_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297111_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 21:13:07.09 +46:46:12.1 in Gaia DR2 blend (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=11.63, BLEND_MAG_FAINT_SEARCH_LIMIT=, VIZIER_COMMAND=#lib/vizquery -site=vizier.china-vo.org -mime=text -source=I/345/gaia2 -out.max=3 -out.add=_r -out.form=mini -sort=Gmag Gmag=0.0..12.61 -c=21:13:07.09 +46:46:12.1 -c.rs=14.75 -out=Source,RA_ICRS,DE_ICRS,Gmag,RPmag,Var#)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297112_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297112_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297112_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297112_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297112_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297115_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297115_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 21:37:16.79 +48:20:17.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297117_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297117_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (104.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297118_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297118_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297118_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297118_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297118_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297119_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297119_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297119_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297119_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297119_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297120_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297120_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 21:29:03.36 +51:14:19.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297122_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297122_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297122_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297122_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297122_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297123_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297123_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297123_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297123_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297123_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297124_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297124_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297126_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297126_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297127_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297127_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297127_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297127_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297127_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297128_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297128_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297128_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297128_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297128_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297129_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297129_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (98.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297131_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297131_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297131_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297131_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297131_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297133_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297133_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297133_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297133_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297133_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297134_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297134_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (278.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297139_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297139_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297139_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297139_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297139_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297142_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297142_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (176.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297144_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297144_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297144_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297144_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297144_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297145_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297145_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 21:31:00.70 +47:48:29.7 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297146_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297146_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297146_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297146_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297146_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297147_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297147_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297148_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297148_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297148_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297148_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297148_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297151_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297151_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (138.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297152_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297152_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297154_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297154_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (564.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297155_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297155_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297155_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297155_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297155_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297156_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297156_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297156_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297156_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297156_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297157_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297157_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297157_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297157_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297157_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297160_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297160_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297160_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297160_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297160_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297161_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297161_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297161_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297161_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297161_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297164_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297164_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (357.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297166_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297166_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297166_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297166_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297166_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297169_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297169_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (211.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297171_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297171_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297171_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297171_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297171_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297172_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297172_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297172_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297172_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297172_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297174_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297174_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297174_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297174_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297174_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297175_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297175_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (108.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297176_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297176_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297176_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297176_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297176_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297177_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297177_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297178_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297178_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 21:49:08.51 +47:07:30.4 in Gaia DR2 blend (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.63, BLEND_MAG_FAINT_SEARCH_LIMIT=, VIZIER_COMMAND=#lib/vizquery -site=vizier.china-vo.org -mime=text -source=I/345/gaia2 -out.max=3 -out.add=_r -out.form=mini -sort=Gmag Gmag=0.0..13.61 -c=21:49:08.51 +47:07:30.4 -c.rs=14.75 -out=Source,RA_ICRS,DE_ICRS,Gmag,RPmag,Var#)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297181_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297181_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 21:48:09.60 +47:19:35.5 in Gaia DR2 blend (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.59, BLEND_MAG_FAINT_SEARCH_LIMIT=, VIZIER_COMMAND=#lib/vizquery -site=vizier.china-vo.org -mime=text -source=I/345/gaia2 -out.max=3 -out.add=_r -out.form=mini -sort=Gmag Gmag=0.0..13.57 -c=21:48:09.60 +47:19:35.5 -c.rs=14.75 -out=Source,RA_ICRS,DE_ICRS,Gmag,RPmag,Var#)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297183_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297183_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (25.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297184_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297184_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297184_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297184_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297184_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297185_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297185_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297185_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297185_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297185_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297186_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297186_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297186_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297186_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297186_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297190_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297190_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297190_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297190_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297190_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297192_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297192_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297192_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297192_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297192_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297193_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297193_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (60.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297195_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297195_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297197_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297197_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (179.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297199_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297199_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297199_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297199_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297199_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297200_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297200_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (81.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297201_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297201_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297201_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297201_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297201_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297202_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297202_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297202_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297202_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297202_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297204_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297204_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (229.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297209_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297209_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297209_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297209_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297209_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297212_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297212_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297212_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297212_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297212_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297213_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297213_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297213_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297213_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297213_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297214_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297214_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297214_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297214_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297214_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297215_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297215_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297216_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297216_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297217_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297217_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297217_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297217_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297217_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297218_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297218_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (457.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297219_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297219_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (504.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297220_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297220_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297220_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297220_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297220_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297222_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297222_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297222_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297222_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297222_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297225_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297225_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297225_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297225_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297225_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297226_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297226_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297226_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297226_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297226_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297227_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297227_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297228_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297228_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (185.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297230_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297230_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297230_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297230_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297230_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297234_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297234_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (181.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297235_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297235_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297235_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297235_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297235_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297236_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297236_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297236_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297236_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297236_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297237_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297237_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297238_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297238_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297238_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297238_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297238_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297239_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297239_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297240_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297240_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297240_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297240_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297240_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297241_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297241_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297242_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297242_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297242_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297242_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297242_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297243_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297243_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297243_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297243_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297243_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297244_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297244_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (315.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297245_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297245_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297246_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297246_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297248_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297248_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297248_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297248_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297248_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297249_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297249_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297249_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297249_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297249_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297251_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297251_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297251_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297251_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297251_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297252_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297252_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297252_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297252_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297252_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297253_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297253_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (430.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297255_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297255_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297255_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297255_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297255_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297258_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297258_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297260_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297260_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (276.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297261_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297261_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297261_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297261_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297261_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297262_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297262_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297262_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297262_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297262_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297263_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297263_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 22:20:11.16 +49:29:00.1 in Gaia DR2 blend (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.00, BLEND_MAG_FAINT_SEARCH_LIMIT=, VIZIER_COMMAND=#lib/vizquery -site=vizier.china-vo.org -mime=text -source=I/345/gaia2 -out.max=3 -out.add=_r -out.form=mini -sort=Gmag Gmag=0.0..13.98 -c=22:20:11.16 +49:29:00.1 -c.rs=14.75 -out=Source,RA_ICRS,DE_ICRS,Gmag,RPmag,Var#)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297265_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297265_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297267_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297267_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297267_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297267_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297267_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297268_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297268_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297268_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297268_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297268_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297269_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297269_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297269_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297269_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297269_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297271_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297271_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (175.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297273_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297273_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297273_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297273_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297273_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297274_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297274_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (390.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297276_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297276_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297277_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297277_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297278_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297278_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297278_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297278_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297278_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297279_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297279_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297279_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297279_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297279_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297280_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297280_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (177.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297284_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297284_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297285_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297285_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297285_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297285_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297285_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297287_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297287_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297287_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297287_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297287_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297288_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297288_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297288_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297288_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297288_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297290_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297290_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297290_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297290_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297290_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297291_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297291_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297291_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297291_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297291_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297292_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297292_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297294_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297294_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297294_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297294_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297294_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297298_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297298_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (104.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297299_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297299_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297300_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297300_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297301_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297301_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (612.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297302_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297302_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 21:38:00.24 +48:43:35.1 in Gaia DR2 blend (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.15, BLEND_MAG_FAINT_SEARCH_LIMIT=, VIZIER_COMMAND=#lib/vizquery -site=vizier.china-vo.org -mime=text -source=I/345/gaia2 -out.max=3 -out.add=_r -out.form=mini -sort=Gmag Gmag=0.0..14.13 -c=21:38:00.24 +48:43:35.1 -c.rs=14.75 -out=Source,RA_ICRS,DE_ICRS,Gmag,RPmag,Var#)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297303_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297303_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297305_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297305_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (49.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297307_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297307_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297308_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297308_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297310_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297310_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297310_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297310_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297310_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297311_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297311_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297312_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297312_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297313_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297313_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (214.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297315_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297315_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (39.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297317_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297317_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297317_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297317_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297317_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297318_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297318_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297318_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297318_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297318_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297322_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297322_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (850.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297325_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297325_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 21:10:07.84 +45:30:36.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297326_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297326_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297326_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297326_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297326_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297327_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297327_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297327_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297327_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297327_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297328_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297328_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (46.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297329_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297329_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297329_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297329_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297329_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297330_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297330_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297332_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297332_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297332_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297332_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297332_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297333_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297333_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (27.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297335_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297335_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297335_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297335_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297335_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297336_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297336_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297337_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297337_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (44.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297341_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297341_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297341_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297341_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297341_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297342_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297342_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297342_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297342_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297342_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297343_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297343_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297344_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297344_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (148.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297346_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297346_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (33.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297347_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297347_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297348_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297348_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297348_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297348_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297348_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297349_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297349_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297349_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297349_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297349_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297351_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297351_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 21:32:51.24 +46:53:28.3 in Gaia DR2 blend (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.23, BLEND_MAG_FAINT_SEARCH_LIMIT=, VIZIER_COMMAND=#lib/vizquery -site=vizier.china-vo.org -mime=text -source=I/345/gaia2 -out.max=3 -out.add=_r -out.form=mini -sort=Gmag Gmag=0.0..14.21 -c=21:32:51.24 +46:53:28.3 -c.rs=14.75 -out=Source,RA_ICRS,DE_ICRS,Gmag,RPmag,Var#)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297352_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297352_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297353_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297353_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297353_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297353_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297353_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297354_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297354_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297354_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297354_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297354_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297355_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297355_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297356_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297356_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297358_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297358_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (711.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297359_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297359_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (141.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297360_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297360_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297362_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297362_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297363_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297363_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297363_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297363_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297363_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297364_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297364_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (51.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297366_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297366_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297366_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297366_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297366_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297367_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297367_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297368_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297368_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297368_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297368_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297368_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297370_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297370_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297370_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297370_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297370_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297373_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297373_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297374_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297374_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (15.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297376_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297376_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297376_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297376_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297376_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297379_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297379_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297383_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297383_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297383_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297383_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297383_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297384_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297384_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (691.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297386_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297386_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297389_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297389_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297390_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297390_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297391_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297391_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (809.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297392_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297392_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297392_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297392_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297392_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297394_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297394_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297394_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297394_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297394_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297395_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297395_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (204.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297396_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297396_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297396_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297396_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297396_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297397_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297397_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297399_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297399_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297399_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297399_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297399_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297400_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297400_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (398.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297402_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297402_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (383.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297403_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297403_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297403_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297403_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297403_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297404_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297404_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297404_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297404_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297404_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297405_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297405_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297407_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297407_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297407_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297407_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297407_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297408_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297408_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297408_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297408_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297408_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297410_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297410_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297413_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297413_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297413_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297413_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297413_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297414_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297414_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297415_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297415_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297416_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297416_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (141.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297419_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297419_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297420_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297420_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297420_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297420_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297420_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297421_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297421_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297421_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297421_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297421_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297422_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297422_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297422_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297422_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297422_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297423_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297423_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297423_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297423_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297423_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297425_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297425_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297425_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297425_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297425_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297427_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297427_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297430_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297430_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (18.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297434_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297434_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297435_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297435_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297436_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297436_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297436_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297436_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297436_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297438_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297438_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297438_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297438_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297438_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297439_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297439_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297439_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297439_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297439_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297440_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297440_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297443_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297443_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297443_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297443_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297443_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297444_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297444_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297445_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297445_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297447_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297447_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297449_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297449_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (806.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297450_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297450_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (175.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297451_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297451_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297452_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297452_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (149.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297453_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297453_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297453_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297453_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297453_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297454_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297454_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297455_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297455_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297455_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297455_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297455_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297457_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297457_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (105.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297459_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297459_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (121.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297460_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297460_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297461_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297461_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297462_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297462_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297462_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297462_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297462_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297463_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297463_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297464_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297464_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297468_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297468_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297468_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297468_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297468_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297469_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297469_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297469_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297469_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297469_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297471_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297471_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297473_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297473_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297473_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297473_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297473_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297474_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297474_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297474_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297474_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297474_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297475_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297475_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297475_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297475_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297475_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297476_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297476_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297476_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297476_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297476_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297477_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297477_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297481_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297481_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297481_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297481_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297481_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297482_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297482_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297483_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297483_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (127.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297484_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297484_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297484_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297484_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297484_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297487_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297487_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297488_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297488_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297489_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297489_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297490_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297490_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297490_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297490_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297490_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297491_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297491_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (94.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297494_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297494_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (128.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297496_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297496_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297496_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297496_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297496_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297497_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297497_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297498_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297498_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (13.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297501_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297501_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297501_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297501_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297501_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297503_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297503_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297504_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297504_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297505_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297505_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297505_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297505_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297505_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297507_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297507_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (415.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297509_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297509_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (46.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297510_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297510_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (36.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297511_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297511_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297511_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297511_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297511_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297512_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297512_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (13.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297514_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297514_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297514_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297514_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297514_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297517_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297517_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297517_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297517_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297517_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297519_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297519_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (150.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297520_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297520_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297520_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297520_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297520_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297522_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297522_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297523_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297523_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (454.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297526_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297526_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297528_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297528_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (235.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297530_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297530_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297532_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297532_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297533_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297533_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297533_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297533_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297533_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297534_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297534_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297535_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297535_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (577.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297536_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297536_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297536_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297536_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297536_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297538_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297538_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297538_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297538_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297538_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297539_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297539_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297539_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297539_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297539_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297540_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297540_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297540_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297540_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297540_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297541_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297541_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297541_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297541_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297541_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297542_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297542_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (15.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297543_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297543_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297544_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297544_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297546_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297546_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297547_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297547_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297548_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297548_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 21:28:10.41 +47:08:12.2 in Gaia DR2 blend (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.59, BLEND_MAG_FAINT_SEARCH_LIMIT=, VIZIER_COMMAND=#lib/vizquery -site=vizier.china-vo.org -mime=text -source=I/345/gaia2 -out.max=3 -out.add=_r -out.form=mini -sort=Gmag Gmag=0.0..14.57 -c=21:28:10.41 +47:08:12.2 -c.rs=14.75 -out=Source,RA_ICRS,DE_ICRS,Gmag,RPmag,Var#)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297554_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297554_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (426.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297556_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297556_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297557_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297557_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297559_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297559_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297560_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297560_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (453.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297562_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297562_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 21:02:53.01 +45:49:44.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297563_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297563_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (13.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297565_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297565_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (55.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297566_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297566_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297568_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297568_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297568_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297568_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297568_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297570_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297570_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (25.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297571_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297571_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297572_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297572_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297573_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297573_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297573_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297573_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297573_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297574_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297574_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (52.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297575_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297575_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297577_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297577_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297579_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297579_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297582_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297582_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297583_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297583_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297584_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297584_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (73.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297585_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297585_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297586_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297586_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297590_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297590_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297592_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297592_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297592_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297592_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297592_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297599_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297599_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (117.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297602_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297602_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (310.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297603_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297603_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297606_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297606_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (346.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297607_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297607_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297608_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297608_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297610_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297610_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297610_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297610_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297610_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297611_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297611_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297611_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297611_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297611_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297615_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297615_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297616_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297616_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297616_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297616_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297616_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297618_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297618_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297620_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297620_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297620_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297620_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297620_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297621_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297621_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297624_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297624_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (356.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297626_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297626_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297627_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297627_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297627_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297627_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297627_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297628_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297628_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (105.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297629_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297629_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297631_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297631_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (348.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297632_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297632_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297633_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297633_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (77.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297634_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297634_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297634_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297634_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297634_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297635_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297635_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297636_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297636_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (55.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297637_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297637_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (144.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297639_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297639_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297639_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297639_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297639_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297640_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297640_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297641_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297641_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (491.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297642_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297642_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297643_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297643_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297643_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297643_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297643_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297645_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297645_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297645_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297645_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297645_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297646_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297646_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297647_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297647_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (237.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297648_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297648_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297649_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297649_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297650_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297650_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (102.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297651_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297651_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (13.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297652_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297652_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (515.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297653_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297653_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297653_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297653_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297653_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297654_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297654_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (79.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297656_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297656_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297657_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297657_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297660_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297660_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (234.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297661_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297661_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297661_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297661_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297661_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297663_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297663_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (84.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297664_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297664_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (497.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297665_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297665_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297668_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297668_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (15.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297671_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297671_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297673_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297673_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297676_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297676_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297677_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297677_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297680_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297680_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297682_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297682_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297684_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297684_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297684_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297684_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297684_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297685_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297685_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297686_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297686_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297686_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297686_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297686_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297687_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297687_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (463.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297688_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297688_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (181.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297689_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297689_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297690_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297690_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (25.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297691_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297691_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297693_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297693_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297695_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297695_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297696_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297696_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297698_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297698_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (178.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297700_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297700_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297701_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297701_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (144.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297702_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297702_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297706_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297706_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297708_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297708_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297708_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297708_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297708_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297709_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297709_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297709_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297709_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297709_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297710_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297710_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297711_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297711_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297711_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297711_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297711_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297712_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297712_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (673.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297714_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297714_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297715_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297715_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297717_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297717_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297717_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297717_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297717_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297720_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297720_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297721_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297721_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297722_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297722_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297727_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297727_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297733_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297733_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297734_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297734_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297735_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297735_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (24.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297736_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297736_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297739_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297739_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297743_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297743_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297743_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297743_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297743_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297744_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297744_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297750_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297750_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297750_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297750_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297750_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297752_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297752_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297752_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297752_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297752_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297753_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297753_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (90.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297756_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297756_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297757_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297757_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (113.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297759_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297759_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297761_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297761_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297763_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297763_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297766_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297766_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297766_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297766_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297766_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297769_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297769_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297770_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297770_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (155.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297771_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297771_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (169.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297772_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297772_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (75.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297773_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297773_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297775_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297775_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (92.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297778_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297778_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297778_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297778_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297778_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297779_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297779_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297780_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297780_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297781_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297781_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297783_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297783_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297784_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297784_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297785_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297785_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297787_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297787_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297790_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297790_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297790_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297790_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297790_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297791_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297791_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (306.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297792_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297792_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297792_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297792_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297792_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297793_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297793_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297794_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297794_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297794_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297794_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297794_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297796_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297796_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297797_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297797_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (134.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297798_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297798_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297800_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297800_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297800_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297800_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297800_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297802_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297802_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297802_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297802_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297802_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297803_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297803_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (456.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297804_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297804_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297805_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297805_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297806_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297806_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297806_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297806_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297806_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297808_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297808_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (129.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297809_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297809_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297811_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297811_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297813_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297813_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297814_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297814_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297814_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297814_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297814_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297815_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297815_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (27.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297816_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297816_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297817_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297817_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297819_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297819_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297820_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297820_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297821_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297821_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297823_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297823_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297825_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297825_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297826_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297826_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (401.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297827_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297827_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (754.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297829_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297829_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297829_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297829_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297829_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297830_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297830_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297832_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297832_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297835_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297835_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (105.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297837_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297837_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297837_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297837_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297837_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297838_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297838_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297840_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297840_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297842_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297842_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297843_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297843_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (26.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297846_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297846_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (141.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297847_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297847_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297848_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297848_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (331.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297849_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297849_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297852_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297852_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297854_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297854_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297855_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297855_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (18.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297858_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297858_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (173.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297861_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297861_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (153.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297862_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297862_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297863_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297863_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (882.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297864_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297864_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (76.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297867_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297867_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (29.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297868_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297868_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (378.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297869_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297869_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297869_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297869_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297869_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297871_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297871_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297873_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297873_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297874_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297874_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297875_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297875_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297875_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297875_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297875_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297877_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297877_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (300.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297878_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297878_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297879_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297879_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (439.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297880_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297880_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (13.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297881_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297881_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297882_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297882_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297883_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297883_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (314.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297886_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297886_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (15.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297892_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297892_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 21:53:27.90 +49:54:16.0 in Gaia DR2 blend (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.94, BLEND_MAG_FAINT_SEARCH_LIMIT=, VIZIER_COMMAND=#lib/vizquery -site=vizier.china-vo.org -mime=text -source=I/345/gaia2 -out.max=3 -out.add=_r -out.form=mini -sort=Gmag Gmag=0.0..14.92 -c=21:53:27.90 +49:54:16.0 -c.rs=14.75 -out=Source,RA_ICRS,DE_ICRS,Gmag,RPmag,Var#)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297893_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297893_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (22.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297894_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297894_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297894_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297894_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297894_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297898_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297898_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297899_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297899_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297899_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297899_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297899_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297903_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297903_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297903_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297903_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297903_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297908_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297908_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297909_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297909_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (32.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297910_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297910_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (137.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297911_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297911_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (904.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297914_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297914_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297914_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297914_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297914_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297916_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297916_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297916_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297916_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297916_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297920_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297920_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297920_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297920_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297920_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297922_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297922_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297923_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297923_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297923_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297923_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297923_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297928_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297928_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (33.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297930_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297930_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (468.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297931_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297931_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (16.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297934_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297934_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (138.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297935_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297935_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (101.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297937_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297937_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (584.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297943_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297943_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297944_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297944_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297945_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297945_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297946_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297946_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297947_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297947_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297948_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297948_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (686.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297949_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297949_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297951_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297951_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297951_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297951_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297951_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297953_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297953_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297954_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297954_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (18.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297956_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297956_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (258.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297959_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297959_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (317.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297964_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297964_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (200.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297965_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297965_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (27.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297966_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297966_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297967_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297967_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (13.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297968_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297968_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297970_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297970_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297973_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297973_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (15.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297974_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297974_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297974_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297974_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297974_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297981_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297981_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297984_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297984_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297985_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297985_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297987_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297987_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297990_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297990_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297992_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297992_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297992_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297992_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297992_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297993_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297993_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297993_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297993_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297993_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297995_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297995_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297996_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297996_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297996_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297996_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297996_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297997_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297997_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297998_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 297998_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (521.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297999_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 297999_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/297999_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/297999_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/297999_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298004_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298004_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (575.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298005_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298005_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298007_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298007_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (695.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298008_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298008_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (119.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298009_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 298009_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/298009_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/298009_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/298009_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298010_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298010_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (16.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298011_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298011_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (382.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298012_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298012_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (47.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298015_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298015_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298017_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298017_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298018_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298018_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298020_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298020_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298021_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298021_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298022_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298022_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298024_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298024_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (26.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298025_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298025_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298026_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298026_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298027_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298027_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298028_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298028_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298029_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298029_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (742.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298030_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 298030_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/298030_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/298030_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/298030_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298032_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298032_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (239.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298033_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298033_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298035_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298035_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298036_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298036_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298038_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298038_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298040_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298040_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298041_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298041_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (319.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298042_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298042_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (17.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298043_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298043_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (222.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298044_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298044_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (22.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298047_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 298047_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/298047_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/298047_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/298047_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298049_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298049_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298050_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298050_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298052_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298052_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298053_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298053_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298056_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298056_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298057_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298057_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298058_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298058_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298062_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298062_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (454.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298063_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298063_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (150.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298069_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298069_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298070_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298070_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298071_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298071_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (13.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298073_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298073_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298075_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298075_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298079_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298079_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298080_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298080_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (556.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298084_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 298084_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/298084_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/298084_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/298084_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298085_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298085_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (95.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298086_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298086_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298087_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298087_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298091_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 298091_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/298091_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/298091_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/298091_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298094_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298094_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298097_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298097_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298100_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298100_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (97.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298103_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298103_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (389.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298104_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298104_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298105_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298105_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298107_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298107_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (26.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298110_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 298110_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/298110_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/298110_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/298110_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298114_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298114_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298116_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 298116_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/298116_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/298116_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/298116_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298117_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 298117_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/298117_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/298117_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/298117_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298119_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298119_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (74.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298120_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298120_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298121_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298121_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298122_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298122_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298124_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298124_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (798.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298125_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 298125_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/298125_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/298125_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/298125_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298126_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298126_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298129_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298129_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (13.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298131_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 298131_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/298131_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/298131_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/298131_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298133_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298133_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (13.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298135_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298135_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298136_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298136_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298137_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 298137_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/298137_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/298137_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/298137_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298138_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298138_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (98.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298139_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 298139_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/298139_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/298139_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/298139_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298140_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298140_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (552.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298142_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 298142_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/298142_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/298142_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/298142_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298144_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298144_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298145_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298145_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298146_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298146_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298148_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298148_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298149_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298149_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (34.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298150_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298150_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (14.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298156_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298156_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298157_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298157_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298158_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298158_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298159_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 298159_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/298159_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/298159_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/298159_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298160_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 298160_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/298160_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/298160_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/298160_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298164_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 298164_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/298164_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/298164_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/298164_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298167_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298167_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298170_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298170_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (13.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298171_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298171_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (73.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298173_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298173_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298175_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298175_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298177_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298177_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (15.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298180_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298180_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298181_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298181_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298182_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 298182_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/298182_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/298182_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/298182_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298183_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298183_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298188_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298188_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298191_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298191_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298195_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298195_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (84.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298200_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298200_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298201_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298201_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298205_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298205_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (13.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298207_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298207_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (713.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298208_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298208_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298209_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298209_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (88.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298210_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298210_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (622.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298211_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298211_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (13.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298212_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298212_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298214_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298214_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (13.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298217_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298217_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298219_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298219_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298220_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298220_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (190.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298222_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298222_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298225_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298225_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 22:06:09.47 +50:41:57.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298229_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298229_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298230_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298230_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (15.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298232_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298232_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (50.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298233_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298233_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (23.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298236_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298236_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298237_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298237_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298239_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298239_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (171.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298240_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298240_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (44.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298242_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298242_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (506.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298245_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 298245_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/298245_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/298245_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/298245_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298247_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 298247_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/298247_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/298247_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/298247_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298248_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298248_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298249_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298249_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298250_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298250_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298251_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 298251_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/298251_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/298251_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/298251_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298255_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298255_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298257_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298257_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298258_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 298258_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/298258_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/298258_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/298258_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298259_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298259_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298260_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298260_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 22:05:45.66 +48:11:58.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298262_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298262_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298263_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298263_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298268_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298268_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (145.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298269_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298269_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298272_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298272_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (16.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298273_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298273_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298276_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298276_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298277_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298277_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298278_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 298278_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/298278_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/298278_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/298278_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298279_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298279_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (43.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298281_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298281_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298283_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298283_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (13.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298284_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298284_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (281.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298286_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298286_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298287_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298287_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298289_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 298289_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/298289_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/298289_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/298289_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298290_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298290_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (232.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298292_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298292_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (140.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298294_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298294_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298295_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298295_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298307_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298307_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298308_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298308_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (13.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298310_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 298310_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/298310_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/298310_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/298310_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298312_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298312_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298314_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298314_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 21:38:29.63 +46:00:17.6 in Gaia DR2 blend (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.16, BLEND_MAG_FAINT_SEARCH_LIMIT=, VIZIER_COMMAND=#lib/vizquery -site=vizier.china-vo.org -mime=text -source=I/345/gaia2 -out.max=3 -out.add=_r -out.form=mini -sort=Gmag Gmag=0.0..15.14 -c=21:38:29.63 +46:00:17.6 -c.rs=14.75 -out=Source,RA_ICRS,DE_ICRS,Gmag,RPmag,Var#)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298315_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298315_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298317_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298317_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298320_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298320_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298323_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298323_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (512.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298324_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298324_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298325_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298325_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298326_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 298326_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/298326_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/298326_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/298326_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298328_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298328_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298332_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298332_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298333_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298333_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (34.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298335_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 298335_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/298335_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/298335_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/298335_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298336_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 298336_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/298336_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/298336_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/298336_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298338_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298338_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298340_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298340_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298342_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298342_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298344_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298344_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298347_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298347_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (21.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298348_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298348_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298349_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298349_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298350_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298350_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298354_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298354_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (44.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298359_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298359_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298361_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298361_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (18.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298363_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298363_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (16.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298364_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 298364_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/298364_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/298364_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/298364_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298368_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298368_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298369_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298369_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298370_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 298370_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/298370_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/298370_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/298370_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298375_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298375_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298376_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 298376_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/298376_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/298376_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/298376_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298379_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298379_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298380_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298380_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298381_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298381_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298383_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 298383_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/298383_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/298383_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/298383_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298389_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298389_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (33.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298394_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298394_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298395_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298395_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298396_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298396_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298401_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298401_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298406_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 298406_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/298406_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/298406_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/298406_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298408_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298408_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (688.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298410_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 298410_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/298410_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/298410_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/298410_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298412_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 298412_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/298412_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/298412_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/298412_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298413_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298413_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298414_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 298414_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/298414_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/298414_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/298414_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298415_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298415_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298419_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298419_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298420_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298420_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (404.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298422_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298422_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298423_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298423_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298424_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298424_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298425_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298425_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (16.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298427_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298427_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298428_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298428_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298431_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298431_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (14.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298434_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298434_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (87.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298435_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298435_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298436_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298436_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298438_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298438_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298440_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298440_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298447_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298447_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298448_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298448_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298451_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298451_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298452_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 298452_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/298452_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/298452_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/298452_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298454_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298454_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (13.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298455_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298455_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298456_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298456_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298457_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298457_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298459_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298459_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298461_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298461_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298462_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298462_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (14.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298464_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298464_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298466_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298466_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (16.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298469_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298469_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298477_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298477_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298478_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298478_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298481_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298481_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (49.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298482_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298482_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (490.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298486_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298486_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298489_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 298489_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/298489_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/298489_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/298489_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298490_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298490_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298493_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298493_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298499_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298499_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (13.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298500_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298500_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298507_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298507_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298513_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298513_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298514_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 298514_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/298514_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/298514_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/298514_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298515_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298515_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298517_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298517_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298522_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298522_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298523_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298523_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (49.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298527_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298527_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298528_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298528_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (126.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298531_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298531_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298535_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298535_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298536_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298536_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298539_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 298539_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/298539_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/298539_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/298539_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298540_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298540_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (15.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298542_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298542_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (27.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298544_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 298544_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/298544_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/298544_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/298544_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298546_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298546_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298547_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 298547_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/298547_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/298547_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/298547_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298551_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298551_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298552_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298552_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298553_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298553_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 21:32:35.45 +48:59:59.9 in Gaia DR2 blend (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.43, BLEND_MAG_FAINT_SEARCH_LIMIT=, VIZIER_COMMAND=#lib/vizquery -site=vizier.china-vo.org -mime=text -source=I/345/gaia2 -out.max=3 -out.add=_r -out.form=mini -sort=Gmag Gmag=0.0..15.41 -c=21:32:35.45 +48:59:59.9 -c.rs=14.75 -out=Source,RA_ICRS,DE_ICRS,Gmag,RPmag,Var#)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298554_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 298554_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/298554_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/298554_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/298554_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298558_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298558_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298560_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298560_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298562_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298562_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (744.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298564_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298564_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298565_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 298565_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/298565_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/298565_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/298565_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298566_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298566_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (292.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298569_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298569_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (13.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298572_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298572_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298573_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 298573_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/298573_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/298573_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/298573_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298575_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298575_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298576_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298576_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (15.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298578_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298578_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (151.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298579_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298579_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298584_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298584_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298586_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298586_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (51.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298589_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298589_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298590_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298590_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298591_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298591_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (16.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298596_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298596_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298598_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 298598_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/298598_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/298598_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/298598_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298599_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298599_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298600_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298600_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (14.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298604_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298604_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298606_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298606_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298609_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298609_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298610_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298610_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298613_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298613_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (17.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298615_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298615_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298617_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298617_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (52.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298619_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298619_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (99.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298620_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298620_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (31.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298623_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298623_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (15.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298633_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298633_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (14.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298635_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298635_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (299.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298636_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298636_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (15.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298638_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298638_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298653_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298653_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298655_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298655_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (14.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298658_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298658_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298659_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 298659_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/298659_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/298659_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/298659_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298660_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298660_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298661_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298661_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (13.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298669_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298669_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298671_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298671_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298672_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298672_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298674_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298674_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298680_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298680_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (71.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298682_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 298682_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/298682_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/298682_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/298682_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298684_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298684_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 22:03:07.60 +49:47:57.5 in Gaia DR2 blend (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.31, BLEND_MAG_FAINT_SEARCH_LIMIT=, VIZIER_COMMAND=#lib/vizquery -site=vizier.china-vo.org -mime=text -source=I/345/gaia2 -out.max=3 -out.add=_r -out.form=mini -sort=Gmag Gmag=0.0..15.29 -c=22:03:07.60 +49:47:57.5 -c.rs=14.75 -out=Source,RA_ICRS,DE_ICRS,Gmag,RPmag,Var#)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298693_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298693_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (71.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298697_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298697_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (659.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298698_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298698_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298702_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 298702_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/298702_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/298702_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/298702_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298715_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298715_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298717_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 298717_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/298717_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/298717_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/298717_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298718_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 298718_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/298718_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/298718_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/298718_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298719_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298719_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298732_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298732_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298735_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298735_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298740_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 298740_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/298740_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/298740_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/298740_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298745_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298745_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 21:59:57.57 +48:20:47.3 in Gaia DR2 blend (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.47, BLEND_MAG_FAINT_SEARCH_LIMIT=, VIZIER_COMMAND=#lib/vizquery -site=vizier.china-vo.org -mime=text -source=I/345/gaia2 -out.max=3 -out.add=_r -out.form=mini -sort=Gmag Gmag=0.0..15.45 -c=21:59:57.57 +48:20:47.3 -c.rs=14.75 -out=Source,RA_ICRS,DE_ICRS,Gmag,RPmag,Var#)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298747_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298747_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298748_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298748_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298751_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298751_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298753_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298753_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (628.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298772_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298772_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298780_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298780_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298781_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298781_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298794_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298794_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298795_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298795_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298801_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298801_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298803_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298803_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298808_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298808_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298810_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298810_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298816_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298816_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298818_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298818_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298825_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298825_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298826_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298826_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298827_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298827_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298829_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298829_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298831_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298831_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (16.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298832_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298832_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298837_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298837_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (25.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298845_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298845_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298864_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298864_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298867_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298867_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (911.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298869_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298869_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298870_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298870_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298872_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298872_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (15.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298873_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298873_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (97.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298875_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298875_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (15.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298881_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298881_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (88.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298882_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298882_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298891_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298891_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298902_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298902_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (409.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298905_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298905_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298907_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298907_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (16.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298908_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298908_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298911_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298911_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298925_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298925_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (546.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298926_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298926_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298928_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 298928_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/298928_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/298928_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/298928_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298931_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298931_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (579.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298935_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298935_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298942_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 298942_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/298942_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/298942_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/298942_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298945_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298945_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (277.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298951_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298951_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (227.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298965_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298965_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (13.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298966_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298966_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298967_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298967_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (207.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298971_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298971_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298988_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298988_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (15.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298997_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 298997_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (111.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 299004_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 299004_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 299009_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 299009_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 299011_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 299011_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 299012_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 299012_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 299013_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 299013_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 299019_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 299019_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (16.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 299029_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 299029_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 299035_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 299035_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/299035_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/299035_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/299035_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 299069_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 299069_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 299075_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 299075_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 299080_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 299080_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 299083_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 299083_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (15.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 299110_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 299110_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (78.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 299128_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 299128_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 299138_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 299138_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 299157_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 299157_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (13.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 299166_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 299166_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 299178_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 299178_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 299184_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 299184_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 299188_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 299188_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 299239_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 299239_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 299434_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 299434_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (77.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 299467_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 299467_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (83.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35454_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 35454_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/35454_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.png to transient_report/35454_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/35454_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/35454_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery3.png
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.png to transient_report/Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits_preview.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256698_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 256698_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (788.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257870_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 257870_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (674.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52489_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 52489_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 21:52:52.60 +48:57:25.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133171_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 133171_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 21:59:08.26 +45:59:32.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 175496_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 175496_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (78.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 276419_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 276419_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (654.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253508_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 253508_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (769.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 37316_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 37316_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.png to transient_report/37316_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_reference.png
The output file transient_report/Cyg-04-Q1b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits_preview.png already exist
Successfully moved Cyg-04-Q1b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.png to transient_report/37316_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery1.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-19-50_20.00sec_-14.90C_LIGHT_0004.png to transient_report/37316_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery2.png
Successfully moved fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005.png to transient_report/37316_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005_discovery3.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 109251_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 109251_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 22:10:58.18 +46:27:25.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227543_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005
The candidate 227543_fd_Cyg-04-Q1b1x1_2026-01-20_19-20-33_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks