This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0573 Cyg,2461126.9056,10.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0573 Cyg 20260327.4056 10.63CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:08:45.47 +47:24:13.5 ;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-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_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 1970517187099961984,2461126.9056,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1970517187099961984 20260327.4056 13.04CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:28:29.72 +43:32:13.1 ;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-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4056 2461126.9056 13.04 21:27:28.18 +43:54:55.2
88.74392 -5.00651 galactic Cyg Second-epoch detections are separated by 1.9" and 4.3 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 J321.8650+43.9187 | 21:27:28.18 +43:54:55.2 (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 J321.8650+43.9187,2461126.9056,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J321.8650+43.9187 20260327.4056 13.04CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:27:28.18 +43:54:55.2 ;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-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4056 2461126.9056 12.75 21:37:05.51 +47:50:37.9
92.65649 -3.27279 galactic Cyg Second-epoch detections are separated by 4.4" and 3.1 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 J324.2690+47.8443 | 21:37:04.56 +47:50:39.6 (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 J324.2690+47.8443,2461126.9056,12.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J324.2690+47.8443 20260327.4056 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 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:37:05.51 +47:50:37.9 ;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-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4056 2461126.9056 12.71 21:06:35.16 +47:21:32.2
88.66861 0.00920 galactic Cyg Second-epoch detections are separated by 2.8" and 3.9 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 J316.6418+47.3610 | 21:06:35.16 +47:21:32.2 (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 J316.6418+47.3610,2461126.9056,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J316.6418+47.3610 20260327.4056 12.71CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:06:35.16 +47:21:32.2 ;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-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4056 2461126.9056 12.69 21:15:09.21 +48:54:44.7
90.77941 0.02654 galactic Cyg Second-epoch detections are separated by 2.5" and 4.2 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 J318.7947+48.9170 | 21:15:09.21 +48:54:44.7 (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 J318.7947+48.9170,2461126.9056,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J318.7947+48.9170 20260327.4056 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 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:15:09.21 +48:54:44.7 ;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-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_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 1967830118118148864,2461126.9056,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1967830118118148864 20260327.4056 12.47CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:33:24.18 +43:10:54.5 ;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-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_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 1978789328479910912,2461126.9056,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1978789328479910912 20260327.4056 12.47CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:38:31.43 +48:30:05.1 ;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-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4056 2461126.9056 12.31 22:04:56.90 +47:35:01.3
96.13263 -6.43738 galactic Lac Second-epoch detections are separated by 5.0" and 4.4 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 J331.2547+47.5890 | 22:04:56.90 +47:35:18.6 (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 J331.2547+47.5890,2461126.9056,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J331.2547+47.5890 20260327.4056 12.31CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:04:56.90 +47:35:01.3 ;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-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_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 J210708.99+474654.4,2461126.9056,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J210708.99+474654.4 20260327.4056 12.53CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:07:07.61 +47:46:43.8 ;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-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4056 2461126.9056 12.56 21:06:41.60 +47:00:02.0
88.41583 -0.24551 galactic Cyg Second-epoch detections are separated by 6.3" and 3.4 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 J316.6669+47.0056 | 21:06:39.36 +46:59:57.3 (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 J316.6669+47.0056,2461126.9056,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J316.6669+47.0056 20260327.4056 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 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:06:41.60 +47:00:02.0 ;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-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_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 J214356.58+472144.7,2461126.9056,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J214356.58+472144.7 20260327.4056 12.47CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:43:55.61 +47:21:47.0 ;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-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4056 2461126.9056 12.43 21:13:14.74 +50:00:06.7
91.35274 1.00344 galactic Cyg Second-epoch detections are separated by 2.1" and 4.0 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 2166098590320405120 | 21:13:15.74 +50:00:13.9 (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 2166098590320405120,2461126.9056,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 2166098590320405120 20260327.4056 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 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:13:14.74 +50:00:06.7 ;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-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_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 1977101371963980672,2461126.9056,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1977101371963980672 20260327.4056 12.20CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:35:51.02 +45:24:27.0 ;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-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4056 2461126.9056 12.45 21:29:10.78 +47:17:36.4
91.30077 -2.77169 galactic Cyg Second-epoch detections are separated by 0.5" and 3.7 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 J322.2961+47.2979 | 21:29:10.78 +47:17:36.4 (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 J322.2961+47.2979,2461126.9056,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J322.2961+47.2979 20260327.4056 12.45CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:29:10.78 +47:17:36.4 ;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-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_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 1979112756697503360,2461126.9056,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1979112756697503360 20260327.4056 12.37CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:38:32.83 +49:46:26.9 ;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-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_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 2162759133008926336,2461126.9056,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 2162759133008926336 20260327.4056 12.62CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:08:24.96 +45:46:08.8 ;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-Q2b1x1_2025-12-26_19-21-50_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4056 2461126.9056 12.81 21:57:15.79 +42:01:08.6
91.61734 -10.02274 galactic Cyg Second-epoch detections are separated by 3.9" and 4.1 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 J329.3064+42.0125 | 21:57:15.79 +42:01:08.6 (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 J329.3064+42.0125,2461126.9056,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J329.3064+42.0125 20260327.4056 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 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:57:15.79 +42:01:08.6 ;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-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_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 J214356.58+472144.7,2461126.9056,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J214356.58+472144.7 20260327.4056 12.13CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:43:56.40 +47:21:45.0 ;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-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4056 2461126.9056 12.49 21:56:13.40 +47:40:53.0
95.01776 -5.46760 galactic Cyg Second-epoch detections are separated by 1.9" and 3.4 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 | Large-amplitude variable Gaia DR2 1976079101026459264 | 21:56:16.49 +47:41:26.6 (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 1976079101026459264,2461126.9056,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1976079101026459264 20260327.4056 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 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:56:13.40 +47:40:53.0 ;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-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_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 J214101.17+435638.9,2461126.9056,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J214101.17+435638.9 20260327.4056 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 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:41:01.96 +43:56:46.0 ;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-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_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
V0619 Cyg,2461126.9056,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0619 Cyg 20260327.4056 12.18CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:31:29.60 +46:25:08.6 ;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-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_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
BH Cyg,2461126.9056,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
BH Cyg 20260327.4056 11.29CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:18:58.01 +41:53:40.3 ;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-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_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
V0411 Cyg,2461126.9056,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0411 Cyg 20260327.4056 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 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:47:07.04 +48:28:58.4 ;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-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4056 2461126.9056 12.78 21:41:57.34 +47:44:04.4
93.19711 -3.89586 galactic Cyg Second-epoch detections are separated by 6.6" and 2.7 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 J325.4927+47.7370 | 21:41:58.27 +47:44:13.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F6 (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 J325.4927+47.7370,2461126.9056,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J325.4927+47.7370 20260327.4056 12.78CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:41:57.34 +47:44:04.4 ;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-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_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
NSVS 5931073,2461126.9056,11.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 5931073 20260327.4056 11.27CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:45:01.52 +44:39:18.6 ;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-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_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
NSVS 5852392,2461126.9056,11.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 5852392 20260327.4056 11.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:16:09.83 +47:29:32.1 ;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-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_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 1977560658587004160,2461126.9056,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1977560658587004160 20260327.4056 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 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:38:24.77 +47:22:55.9 ;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-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_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
NSVS 5850641,2461126.9056,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 5850641 20260327.4056 12.65CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:13:57.54 +48:56:54.7 ;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-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_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
NSVS 5979156,2461126.9056,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 5979156 20260327.4056 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 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:41:23.65 +47:01:13.7 ;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-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_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
NSVS 5925047,2461126.9056,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 5925047 20260327.4056 12.30CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:39:17.08 +42:26:28.3 ;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-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_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
V2074 Cyg,2461126.9056,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V2074 Cyg 20260327.4056 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:43:33.99 +49:08:56.2 ;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-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_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
V0656 Cyg,2461126.9056,12.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0656 Cyg 20260327.4056 12.00CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:45:04.59 +47:54:05.0 ;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-Q2b1x1_2025-12-26_19-21-50_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4056 2461126.9056 12.33 21:33:42.56 +47:16:17.8
91.84795 -3.31211 galactic Cyg Second-epoch detections are separated by 5.1" and 4.7 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 J323.4297+47.2635 | 21:33:43.14 +47:15:48.7 (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 J323.4297+47.2635,2461126.9056,12.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J323.4297+47.2635 20260327.4056 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 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:33:42.56 +47:16:17.8 ;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-Q2b1x1_2025-12-26_19-21-50_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_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
V0644 Cyg,2461126.9056,10.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0644 Cyg 20260327.4056 10.41CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:40:13.05 +45:27:16.2 ;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-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_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 J213538.63+453419.7,2461126.9056,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J213538.63+453419.7 20260327.4056 12.44CV 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 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:35:38.85 +45:34:19.5 ;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-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_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
NSVS 5917693,2461126.9056,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 5917693 20260327.4056 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 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:33:13.75 +44:27:07.8 ;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-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20_00sec_-15_00C_LIGHT_0436_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20_00sec_-14_90C_LIGHT_0435_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461036.55649360 27.12.2025 01:21:11.047 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
First image: 2461036.55649360 27.12.2025 01:21:11.047 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
Last image: 2461126.90590557 27.03.2026 09:44:20.241 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 17
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.07
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: 7 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): 26648
Objects passed selection criteria: 26518
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 19079.5
Average stars matched: 18084.5 (94.785 %)
Memory usage VmPeak: 130184 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Mar 27 05:24:28 CDT 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: 2461036.55649360 27.12.2025 01:21:11.047 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
First image: 2461036.55649360 27.12.2025 01:21:11.047 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
Last image: 2461126.90590557 27.03.2026 09:44:20.241 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 166
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.72
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: 56 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 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): 192119
Objects passed selection criteria: 191578
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 133113
Average stars matched: 125601 (94.3567 %)
Memory usage VmPeak: 1950904 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Mar 27 05:29:29 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_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 --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits
SExtractor catalog cache: saved Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat to cache
SExtractor catalog cache: saved Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.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: 2461126.90532675
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Plate-solving the images
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits exists and is non-empty
Saving wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits to local_wcs_cache/
'wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits' -> 'local_wcs_cache/wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits'
wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits exists and is non-empty
Saving wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits to local_wcs_cache/
'wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits' -> 'local_wcs_cache/wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits'
wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits exists and is non-empty
Saving wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits to local_wcs_cache/
'wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits' -> 'local_wcs_cache/wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits'
wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits exists and is non-empty
Saving wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits to local_wcs_cache/
'wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits' -> 'local_wcs_cache/wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.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 21:35:59.427 +46:00:14.09
Second-epoch image center 21:35:52.663 +45:56:27.20
Angular distance between the image centers 0.07 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 21:35:59.427 +46:00:14.09
Second-epoch image center 21:35:50.965 +45:56:41.83
Angular distance between the image centers 0.06 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 21:35:52.663 +45:56:27.20
Second-epoch second image center 21:35:50.965 +45:56:41.83
Angular distance between the image centers 0.00638 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits &> /tmp/tmp.1s3EifTDaT
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits &> /tmp/tmp.zTyJBGhnPA
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits &> /tmp/tmp.pBRYR6MXez
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits &> /tmp/tmp.sxHyY8wsud
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.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-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits and wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.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-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits and wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat
Found non-empty wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits and wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat
The reference image (wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits) and catalog (wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat) found
'wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.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 14243 out of 30795 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.935356
a=0.000000 b=1.000000 c=22.935356
From vast_summary.log: estimated ref. image limiting mag.: -8.07
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.87
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.87
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 14 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.4 pix Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
2.4 pix Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
4.3 pix fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits
4.7 pix fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits
Limiting magnitude estimates:
14.9 mag. Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
14.9 mag. Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
13.7 mag. fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits
13.5 mag. fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits
All-image limiting magnitude estimate: 13.5 (SNR ) 11.2 (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 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.1s3EifTDaT (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits' -> 'wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
WCS_IMAGE_NAME=wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
WCS-calibrated image found: wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
Checking if the catalog wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat corresponding to the image wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits alredy exist and is non-empty...
Catalog wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat corresponding to the image wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
WCS catalog name: wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3934, passed=30795
Got 30795 stars (including 26843 good ones) from the SExtractor catalog wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat
util/solve_plate_with_UCAC5 got 30795 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 958 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: 0.73"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.66"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.66"
Estimated accuracy of the plate solution: 0.63"
Excluding outliers - 954 stars left (next iteration limit 1049)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits -region wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.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.zTyJBGhnPA (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits' -> 'wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
WCS_IMAGE_NAME=wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
WCS-calibrated image found: wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
Checking if the catalog wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits.cat corresponding to the image wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits alredy exist and is non-empty...
Catalog wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits.cat corresponding to the image wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
WCS catalog name: wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3890, passed=30626
Got 30626 stars (including 26706 good ones) from the SExtractor catalog wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits.cat
util/solve_plate_with_UCAC5 got 30626 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 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: 0.86"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.79"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.78"
Estimated accuracy of the plate solution: 0.67"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits -region wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.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.pBRYR6MXez (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 (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.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=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits
WCS-calibrated image found: wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits
Checking if the catalog wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits.cat corresponding to the image wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits.cat corresponding to the image wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits
WCS catalog name: wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=676, passed=13454
Got 13454 stars (including 12773 good ones) from the SExtractor catalog wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits.cat
util/solve_plate_with_UCAC5 got 13454 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.2'
Seting catalog search parameters based on the expected field of view 939.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013044 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010436 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 942 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: 0.97"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.97"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.97"
Estimated accuracy of the plate solution: 1.10"
Excluding outliers - 933 stars left (next iteration limit 1028)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits -region wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.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.sxHyY8wsud (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 (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.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=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits
WCS-calibrated image found: wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits
Checking if the catalog wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits.cat corresponding to the image wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits.cat corresponding to the image wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits
WCS catalog name: wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=620, passed=11981
Got 11981 stars (including 11358 good ones) from the SExtractor catalog wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits.cat
util/solve_plate_with_UCAC5 got 11981 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.2'
Seting catalog search parameters based on the expected field of view 939.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013044 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010436 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 942 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: 0.94"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.97"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.98"
Estimated accuracy of the plate solution: 1.11"
Excluding outliers - 933 stars left (next iteration limit 1028)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits -region wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.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_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits'
Saving fully-calibrated image wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits'
Saving fully-calibrated image wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits'
Saving fully-calibrated image wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits'
Preparing the HTML report for the field Cyg-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out12359.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 4s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53068_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 53068_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:48:31.62 +42:05:31.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22924_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 22924_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:04:56.92 +43:55:45.3 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11124_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 11124_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:06:37.01 +47:38:53.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05487_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 05487_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:46:47.96 +49:18:36.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18803_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 18803_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:36:02.68 +45:22:28.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18301_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 18301_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:33:59.04 +45:35:30.3 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12359_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
Preparing report for the candidate 12359_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04384_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 04384_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:40:48.73 +49:49:40.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 17410_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 17410_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:42:08.49 +45:45:56.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 15195_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 15195_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:29:27.36 +46:32:29.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24427_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 24427_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:40:11.49 +43:16:28.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07552_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 07552_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:26:52.06 +48:50:08.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23153_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 23153_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:18:27.44 +43:56:47.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18402_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 18402_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 22:06:01.78 +45:00:51.4 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 5s
Prepared the HTML report for the field Cyg-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
21:08:45.47 +47:24:13.5
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits
SExtractor catalog cache: saved Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat to cache
SExtractor catalog cache: saved Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
Creating symlink local_wcs_cache/wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
Creating symlink local_wcs_cache/wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits
Creating symlink local_wcs_cache/wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits
Creating symlink local_wcs_cache/exclusion_list.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-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits exists and is non-empty
wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits exists and is non-empty
wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits exists and is non-empty
wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.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 21:35:59.427 +46:00:14.09
Second-epoch image center 21:35:52.663 +45:56:27.20
Angular distance between the image centers 0.07 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 21:35:59.427 +46:00:14.09
Second-epoch image center 21:35:50.965 +45:56:41.83
Angular distance between the image centers 0.06 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 21:35:52.663 +45:56:27.20
Second-epoch second image center 21:35:50.965 +45:56:41.83
Angular distance between the image centers 0.00638 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits &> /tmp/tmp.6o8ueBciOP
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits &> /tmp/tmp.xFsn3h11R4
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits &> /tmp/tmp.Cj1qaBhF6e
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits &> /tmp/tmp.Ga2s6FCPQL
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.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-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits and wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.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-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits and wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat
Found non-empty wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits and wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat
The reference image (wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits) and catalog (wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat) found
'wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.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 15408 out of 227547 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.745984
a=0.000000 b=1.000000 c=22.745984
From vast_summary.log: estimated ref. image limiting mag.: -7.72
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
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 121 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
2.2 pix Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
4.3 pix fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits
4.7 pix fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits
Limiting magnitude estimates:
15.0 mag. Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
15.0 mag. Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
13.7 mag. fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits
13.6 mag. fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits
All-image limiting magnitude estimate: 13.6 (SNR ) 12.9 (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 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.6o8ueBciOP (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits' -> 'wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
WCS_IMAGE_NAME=wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
WCS-calibrated image found: wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
Checking if the catalog wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat corresponding to the image wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits alredy exist and is non-empty...
Catalog wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat corresponding to the image wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
WCS catalog name: wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=41, blended=44928, passed=227506
Got 227506 stars (including 182305 good ones) from the SExtractor catalog wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat
util/solve_plate_with_UCAC5 got 227506 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 961 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: 0.80"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.73"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.73"
Estimated accuracy of the plate solution: 0.66"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits -region wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.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.xFsn3h11R4 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits' -> 'wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
WCS_IMAGE_NAME=wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
WCS-calibrated image found: wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
Checking if the catalog wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits.cat corresponding to the image wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits alredy exist and is non-empty...
Catalog wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits.cat corresponding to the image wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
WCS catalog name: wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=53, blended=45138, passed=228742
Got 228742 stars (including 183314 good ones) from the SExtractor catalog wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits.cat
util/solve_plate_with_UCAC5 got 228742 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 962 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: 0.88"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.85"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.85"
Estimated accuracy of the plate solution: 0.70"
Excluding outliers - 958 stars left (next iteration limit 1054)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits -region wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.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.Cj1qaBhF6e (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 (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.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=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits
WCS-calibrated image found: wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits
Checking if the catalog wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits.cat corresponding to the image wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits.cat corresponding to the image wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits
WCS catalog name: wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=8737, passed=72948
Got 72948 stars (including 64172 good ones) from the SExtractor catalog wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits.cat
util/solve_plate_with_UCAC5 got 72948 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.2'
Seting catalog search parameters based on the expected field of view 939.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013044 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010436 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 939 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: 0.98"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.92"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.92"
Estimated accuracy of the plate solution: 1.01"
Excluding outliers - 933 stars left (next iteration limit 1028)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits -region wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.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.Ga2s6FCPQL (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 (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.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=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits
WCS-calibrated image found: wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits
Checking if the catalog wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits.cat corresponding to the image wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits.cat corresponding to the image wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits
WCS catalog name: wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=1, no_mag_err=0, low_SNR=8, blended=7981, passed=64525
Got 64525 stars (including 56513 good ones) from the SExtractor catalog wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits.cat
util/solve_plate_with_UCAC5 got 64525 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.2'
Seting catalog search parameters based on the expected field of view 939.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013044 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010436 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 943 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: 0.99"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.96"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.96"
Estimated accuracy of the plate solution: 1.03"
Excluding outliers - 934 stars left (next iteration limit 1029)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits -region wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.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_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
Saving fully-calibrated image wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
Saving fully-calibrated image wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-43-30_20.00sec_-14.90C_LIGHT_0435.fits
Saving fully-calibrated image wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_052143_TTUQ2b1x1_9751_YMvYuRdE/wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436.fits
Preparing the HTML report for the field Cyg-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out150267.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out257959.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out257961.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out257990.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out258004.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out264644.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out113996.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134934.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137859.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out153896.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out161501.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out169996.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out178552.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out217051.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226797.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out240271.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out240373.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out240434.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out257945.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out257946.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out257973.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out257991.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out257995.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out257998.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out258000.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out258001.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out258006.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out258008.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out258010.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out258013.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out262398.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out262888.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out263035.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out43374.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51476.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out58347.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out73421.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77922.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out86368.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out87004.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out87861.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95580.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 37s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 21s
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Considering the candidate 257945_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
Preparing report for the candidate 257945_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
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Considering the candidate 257946_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
Preparing report for the candidate 257946_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
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Considering the candidate 257959_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 257959_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:28:07.93 +48:30:09.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)
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Considering the candidate 257961_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 257961_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:11:17.54 +46:26:44.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 4.570 2164300575272385152 317.82414015447 +46.44468257219 13.4290 13.0087 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.570#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 257973_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
Preparing report for the candidate 257973_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
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Considering the candidate 257990_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 257990_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:32:31.54 +49:26:55.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.69, MAG_FAINT_SEARCH_LIMIT=13.67)
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Considering the candidate 257991_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
Preparing report for the candidate 257991_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
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Considering the candidate 257995_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
Preparing report for the candidate 257995_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
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Considering the candidate 257998_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
Preparing report for the candidate 257998_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
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Considering the candidate 258000_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
Preparing report for the candidate 258000_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
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Considering the candidate 258001_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
Preparing report for the candidate 258001_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
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Considering the candidate 258004_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 258004_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:31:04.12 +47:57:11.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)
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Considering the candidate 258006_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
Preparing report for the candidate 258006_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
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Considering the candidate 258008_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
Preparing report for the candidate 258008_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
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Considering the candidate 258010_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
Preparing report for the candidate 258010_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
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Considering the candidate 258013_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
Preparing report for the candidate 258013_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
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Considering the candidate 261390_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 261390_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 22:05:53.48 +48:16:02.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261422_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 261422_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:41:51.56 +45:45:40.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261537_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 261537_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
Rejecting candidate due to large distance (22.9") between the two second-epoch detections
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Considering the candidate 261694_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 261694_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:15:43.92 +47:57:24.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 262398_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
Preparing report for the candidate 262398_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
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Considering the candidate 262888_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
Preparing report for the candidate 262888_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
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Considering the candidate 263035_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
Preparing report for the candidate 263035_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
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Considering the candidate 263288_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 263288_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:56:53.50 +48:40:29.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 263346_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 263346_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:41:48.44 +45:45:56.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263432_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 263432_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 22:03:42.71 +49:44:21.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263665_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 263665_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 22:11:00.62 +49:04:14.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263784_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 263784_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:27:09.97 +46:52:19.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264307_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 264307_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:49:09.85 +49:42:05.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264630_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 264630_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:39:14.67 +46:09:14.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264644_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 264644_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:38:35.22 +47:44:28.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 4.254 1977621715844950656 324.64803673379 +47.74047306283 12.7794 11.9636 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.254#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 264728_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 264728_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:53:25.86 +42:43:45.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264735_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 264735_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
Rejecting candidate due to large distance (23.0") between the two second-epoch detections
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Considering the candidate 264762_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 264762_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:22:49.25 +46:30:56.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264978_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 264978_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:51:21.81 +44:39:49.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265025_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 265025_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:29:03.34 +47:16:42.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265036_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 265036_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
Rejecting candidate due to large distance (22.9") between the two second-epoch detections
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Considering the candidate 265130_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 265130_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
Rejecting candidate due to large distance (22.9") between the two second-epoch detections
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Considering the candidate 265175_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 265175_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
Rejecting candidate due to large distance (23.5") between the two second-epoch detections
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Considering the candidate 265180_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 265180_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:56:10.29 +48:04:09.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265276_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 265276_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
Rejecting candidate due to large distance (22.4") between the two second-epoch detections
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Considering the candidate 265531_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 265531_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:59:24.50 +48:33:06.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266162_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 266162_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
Rejecting candidate due to large distance (22.7") between the two second-epoch detections
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Considering the candidate 266485_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 266485_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
Rejecting candidate due to large distance (24.1") between the two second-epoch detections
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Considering the candidate 266571_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 266571_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
Rejecting candidate due to large distance (23.5") between the two second-epoch detections
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Considering the candidate 266768_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 266768_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
Rejecting candidate due to large distance (24.4") between the two second-epoch detections
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Considering the candidate 266801_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 266801_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
Rejecting candidate due to large distance (23.5") between the two second-epoch detections
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Considering the candidate 266811_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 266811_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 266844_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 266844_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
Rejecting candidate due to large distance (22.7") between the two second-epoch detections
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Considering the candidate 266923_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 266923_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
Rejecting candidate due to large distance (22.6") between the two second-epoch detections
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Considering the candidate 266939_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 266939_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
Rejecting candidate due to large distance (22.2") between the two second-epoch detections
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Considering the candidate 266957_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 266957_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
Rejecting candidate due to large distance (25.8") between the two second-epoch detections
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Considering the candidate 266984_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 266984_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
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Considering the candidate 267013_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 267013_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
Rejecting candidate due to large distance (22.3") between the two second-epoch detections
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Considering the candidate 240271_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
Preparing report for the candidate 240271_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
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Considering the candidate 50912_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 50912_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 22:03:45.08 +48:26:57.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192707_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 192707_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:20:23.81 +43:18:06.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 130655_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 130655_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:38:32.08 +45:42:46.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 149014_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 149014_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:34:09.14 +44:59:34.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 226797_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
Preparing report for the candidate 226797_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
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Considering the candidate 86368_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
Preparing report for the candidate 86368_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
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Considering the candidate 73421_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
Preparing report for the candidate 73421_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
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Considering the candidate 85272_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 85272_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:40:32.61 +47:26:24.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169996_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
Preparing report for the candidate 169996_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
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Considering the candidate 113996_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
Preparing report for the candidate 113996_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
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Considering the candidate 217051_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
Preparing report for the candidate 217051_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
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Considering the candidate 255695_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 255695_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:22:09.00 +43:32:16.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 89637_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 89637_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:08:45.13 +47:24:10.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 58347_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
Preparing report for the candidate 58347_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
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Considering the candidate 127915_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 127915_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:29:19.99 +45:56:55.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 216586_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 216586_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:11:37.22 +41:51:44.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 77922_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
Preparing report for the candidate 77922_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
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Considering the candidate 153896_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
Preparing report for the candidate 153896_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
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Considering the candidate 171889_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 171889_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:37:14.74 +43:52:39.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 87861_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
Preparing report for the candidate 87861_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
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Considering the candidate 122202_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 122202_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:24:35.11 +46:08:47.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57451_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 57451_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:10:10.43 +48:42:58.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 83186_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 83186_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 22:07:38.24 +47:00:27.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 87004_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
Preparing report for the candidate 87004_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
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Considering the candidate 51476_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
Preparing report for the candidate 51476_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
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Considering the candidate 95580_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
Preparing report for the candidate 95580_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
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Considering the candidate 150267_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 150267_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:01:42.99 +44:55:01.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)
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Considering the candidate 31202_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 31202_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:40:48.72 +49:49:40.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 120491_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 120491_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:58:24.41 +45:52:21.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 178552_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
Preparing report for the candidate 178552_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
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Considering the candidate 61617_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 61617_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:39:39.45 +48:26:29.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 43374_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
Preparing report for the candidate 43374_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
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Considering the candidate 121466_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 121466_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 22:09:04.71 +45:30:27.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 94270_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 94270_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 22:10:57.48 +46:27:26.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 76275_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 76275_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 22:09:38.80 +47:15:05.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 240434_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
Preparing report for the candidate 240434_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 240373_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
Preparing report for the candidate 240373_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 224886_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 224886_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:48:31.60 +42:05:31.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137859_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
Preparing report for the candidate 137859_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134934_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
Preparing report for the candidate 134934_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 161501_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
Preparing report for the candidate 161501_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131667_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 131667_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:33:18.38 +45:51:14.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 146074_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 146074_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:36:03.12 +45:22:29.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 138802_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 138802_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:33:59.32 +45:35:30.6 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134409_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 134409_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:42:08.52 +45:45:56.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 157414_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 157414_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:37:27.93 +44:41:48.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115357_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 115357_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:29:27.45 +46:32:29.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 110364_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 110364_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:25:20.23 +46:42:55.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189554_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 189554_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:40:11.52 +43:16:28.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 169436_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 169436_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:16:17.23 +44:14:19.1 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 36682_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 36682_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:42:38.93 +49:36:00.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 57487_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 57487_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:26:52.09 +48:50:08.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 42539_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 42539_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:46:47.98 +49:18:36.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 174503_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 174503_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:18:27.49 +43:56:48.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 30344_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 30344_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:32:56.77 +49:58:40.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 43891_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 43891_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:22:00.66 +49:23:20.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 180991_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 180991_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:17:23.22 +42:41:02.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 42320_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 42320_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:19:28.82 +49:30:36.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 223368_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 223368_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:16:29.69 +42:15:07.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 148743_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 148743_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 22:02:56.58 +44:38:59.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 96108_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 96108_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 22:05:15.72 +46:44:43.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 139317_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 139317_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 22:06:01.80 +45:00:51.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 157310_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 157310_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:02:24.61 +44:47:29.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 122710_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 122710_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:01:11.00 +46:09:23.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 175379_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 175379_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:04:56.95 +43:55:45.5 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86476_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436
The candidate 86476_fd_Cyg-04-Q2b1x1_2026-03-27_04-44-20_20.00sec_-15.00C_LIGHT_0436 did not pass the final checks
**** FOUND 21:06:36.99 +47:38:54.1 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 10s
make_report_in_HTML.sh TOTAL: 68s
Prepared the HTML report for the field Cyg-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
21:08:45.47 +47:24:13.5
21:31:29.60 +46:25:08.6
21:35:38.85 +45:34:19.5
21:40:13.05 +45:27:16.2
21:45:01.52 +44:39:18.6
21:33:13.75 +44:27:07.8
21:41:01.96 +43:56:46.0
21:39:17.08 +42:26:28.3
21:18:58.01 +41:53:40.3
21:57:15.79 +42:01:08.6
21:08:24.96 +45:46:08.8
21:33:42.56 +47:16:17.8
21:45:04.59 +47:54:05.0
21:28:29.72 +43:32:13.1
21:27:28.18 +43:54:55.2
21:37:05.51 +47:50:37.9
21:06:35.16 +47:21:32.2
21:15:09.21 +48:54:44.7
21:33:24.18 +43:10:54.5
21:38:31.43 +48:30:05.1
22:04:56.90 +47:35:01.3
21:07:07.61 +47:46:43.8
21:06:41.60 +47:00:02.0
21:43:55.61 +47:21:47.0
21:13:14.74 +50:00:06.7
21:35:51.02 +45:24:27.0
21:29:10.78 +47:17:36.4
21:38:32.83 +49:46:26.9
21:43:33.99 +49:08:56.2
21:13:57.54 +48:56:54.7
21:47:07.04 +48:28:58.4
21:56:13.40 +47:40:53.0
21:41:57.34 +47:44:04.4
21:43:56.40 +47:21:45.0
21:38:24.77 +47:22:55.9
21:16:09.83 +47:29:32.1
21:41:23.65 +47:01:13.7
########### Completed Cyg-04-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
21:08:45.47 +47:24:13.5
21:28:29.72 +43:32:13.1
21:27:28.18 +43:54:55.2
21:37:05.51 +47:50:37.9
21:06:35.16 +47:21:32.2
21:15:09.21 +48:54:44.7
21:33:24.18 +43:10:54.5
21:38:31.43 +48:30:05.1
22:04:56.90 +47:35:01.3
21:07:07.61 +47:46:43.8
21:06:41.60 +47:00:02.0
21:43:55.61 +47:21:47.0
21:13:14.74 +50:00:06.7
21:35:51.02 +45:24:27.0
21:29:10.78 +47:17:36.4
21:38:32.83 +49:46:26.9
21:08:24.96 +45:46:08.8
21:57:15.79 +42:01:08.6
21:43:56.40 +47:21:45.0
21:56:13.40 +47:40:53.0
21:41:01.96 +43:56:46.0
21:31:29.60 +46:25:08.6
21:18:58.01 +41:53:40.3
21:47:07.04 +48:28:58.4
21:41:57.34 +47:44:04.4
21:45:01.52 +44:39:18.6
21:16:09.83 +47:29:32.1
21:38:24.77 +47:22:55.9
21:13:57.54 +48:56:54.7
21:41:23.65 +47:01:13.7
21:39:17.08 +42:26:28.3
21:43:33.99 +49:08:56.2
21:45:04.59 +47:54:05.0
21:33:42.56 +47:16:17.8
21:40:13.05 +45:27:16.2
21:35:38.85 +45:34:19.5
21:33:13.75 +44:27:07.8
###################################################################################
21:08:45.47 +47:24:13.5 -- not an asteroid (will add it to exclusion list)
21:28:29.72 +43:32:13.1 -- not an asteroid (will add it to exclusion list)
21:27:28.18 +43:54:55.2 -- not an asteroid (will add it to exclusion list)
21:37:05.51 +47:50:37.9 -- not an asteroid (will add it to exclusion list)
21:06:35.16 +47:21:32.2 -- not an asteroid (will add it to exclusion list)
21:15:09.21 +48:54:44.7 -- not an asteroid (will add it to exclusion list)
21:33:24.18 +43:10:54.5 -- not an asteroid (will add it to exclusion list)
21:38:31.43 +48:30:05.1 -- not an asteroid (will add it to exclusion list)
22:04:56.90 +47:35:01.3 -- not an asteroid (will add it to exclusion list)
21:07:07.61 +47:46:43.8 -- not an asteroid (will add it to exclusion list)
21:06:41.60 +47:00:02.0 -- not an asteroid (will add it to exclusion list)
21:43:55.61 +47:21:47.0 -- not an asteroid (will add it to exclusion list)
21:13:14.74 +50:00:06.7 -- not an asteroid (will add it to exclusion list)
21:35:51.02 +45:24:27.0 -- not an asteroid (will add it to exclusion list)
21:29:10.78 +47:17:36.4 -- not an asteroid (will add it to exclusion list)
21:38:32.83 +49:46:26.9 -- not an asteroid (will add it to exclusion list)
21:08:24.96 +45:46:08.8 -- not an asteroid (will add it to exclusion list)
21:57:15.79 +42:01:08.6 -- not an asteroid (will add it to exclusion list)
21:43:56.40 +47:21:45.0 -- not an asteroid (will add it to exclusion list)
21:56:13.40 +47:40:53.0 -- not an asteroid (will add it to exclusion list)
21:41:01.96 +43:56:46.0 -- not an asteroid (will add it to exclusion list)
21:31:29.60 +46:25:08.6 -- not an asteroid (will add it to exclusion list)
21:18:58.01 +41:53:40.3 -- not an asteroid (will add it to exclusion list)
21:47:07.04 +48:28:58.4 -- not an asteroid (will add it to exclusion list)
21:41:57.34 +47:44:04.4 -- not an asteroid (will add it to exclusion list)
21:45:01.52 +44:39:18.6 -- not an asteroid (will add it to exclusion list)
21:16:09.83 +47:29:32.1 -- not an asteroid (will add it to exclusion list)
21:38:24.77 +47:22:55.9 -- not an asteroid (will add it to exclusion list)
21:13:57.54 +48:56:54.7 -- not an asteroid (will add it to exclusion list)
21:41:23.65 +47:01:13.7 -- not an asteroid (will add it to exclusion list)
21:39:17.08 +42:26:28.3 -- not an asteroid (will add it to exclusion list)
21:43:33.99 +49:08:56.2 -- not an asteroid (will add it to exclusion list)
21:45:04.59 +47:54:05.0 -- not an asteroid (will add it to exclusion list)
21:33:42.56 +47:16:17.8 -- not an asteroid (will add it to exclusion list)
21:40:13.05 +45:27:16.2 -- not an asteroid (will add it to exclusion list)
21:35:38.85 +45:34:19.5 -- not an asteroid (will add it to exclusion list)
21:33:13.75 +44:27:07.8 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
21:06:35.16 +47:21:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:06:41.60 +47:00:02.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:07:07.61 +47:46:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:08:24.96 +45:46:08.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:08:45.47 +47:24:13.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:13:14.74 +50:00:06.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:13:57.54 +48:56:54.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:15:09.21 +48:54:44.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:16:09.83 +47:29:32.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:18:58.01 +41:53:40.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:28.18 +43:54:55.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:29.72 +43:32:13.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:10.78 +47:17:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:29.60 +46:25:08.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:33:13.75 +44:27:07.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:33:24.18 +43:10:54.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:33:42.56 +47:16:17.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:38.85 +45:34:19.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:51.02 +45:24:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:05.51 +47:50:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:38:24.77 +47:22:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:38:31.43 +48:30:05.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:38:32.83 +49:46:26.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:17.08 +42:26:28.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:13.05 +45:27:16.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:01.96 +43:56:46.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:23.65 +47:01:13.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:57.34 +47:44:04.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:33.99 +49:08:56.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:55.61 +47:21:47.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:56.40 +47:21:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:01.52 +44:39:18.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:04.59 +47:54:05.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:47:07.04 +48:28:58.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:13.40 +47:40:53.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:57:15.79 +42:01:08.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:04:56.90 +47:35:01.3 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
21:06:35.16 +47:21:32.2 -- not a known variable star
21:06:41.60 +47:00:02.0 -- not a known variable star
21:07:07.61 +47:46:43.8 -- a known variable star
21:08:24.96 +45:46:08.8 -- a known variable star
21:08:45.47 +47:24:13.5 -- a known variable star
21:13:14.74 +50:00:06.7 -- not a known variable star
21:13:57.54 +48:56:54.7 -- a known variable star
21:15:09.21 +48:54:44.7 -- not a known variable star
21:16:09.83 +47:29:32.1 -- a known variable star
21:18:58.01 +41:53:40.3 -- a known variable star
21:27:28.18 +43:54:55.2 -- not a known variable star
21:28:29.72 +43:32:13.1 -- a known variable star
21:29:10.78 +47:17:36.4 -- not a known variable star
21:31:29.60 +46:25:08.6 -- a known variable star
21:33:13.75 +44:27:07.8 -- a known variable star
21:33:24.18 +43:10:54.5 -- a known variable star
21:33:42.56 +47:16:17.8 -- not a known variable star
21:35:38.85 +45:34:19.5 -- a known variable star
21:35:51.02 +45:24:27.0 -- a known variable star
21:37:05.51 +47:50:37.9 -- not a known variable star
21:38:24.77 +47:22:55.9 -- a known variable star
21:38:31.43 +48:30:05.1 -- a known variable star
21:38:32.83 +49:46:26.9 -- a known variable star
21:39:17.08 +42:26:28.3 -- a known variable star
21:40:13.05 +45:27:16.2 -- a known variable star
21:41:01.96 +43:56:46.0 -- a known variable star
21:41:23.65 +47:01:13.7 -- a known variable star
21:41:57.34 +47:44:04.4 -- not a known variable star
21:43:33.99 +49:08:56.2 -- a known variable star
21:43:55.61 +47:21:47.0 -- a known variable star
21:43:56.40 +47:21:45.0 -- a known variable star
21:45:01.52 +44:39:18.6 -- a known variable star
21:45:04.59 +47:54:05.0 -- a known variable star
21:47:07.04 +48:28:58.4 -- a known variable star
21:56:13.40 +47:40:53.0 -- not a known variable star
21:57:15.79 +42:01:08.6 -- not a known variable star
22:04:56.90 +47:35:01.3 -- not a known variable star
Found 12 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
37 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
###################################################################################
Adding identified Gaia sources from exclusion_list_gaiadr2.txt
exclusion_list_apass.txt NOT FOUND
IS_THIS_TEST_RUN= NO ALLOW_EXCLUSION_LIST_UPDATE= YES
#### Adding the following to the exclusion list ####
21:06:35.16 +47:21:32.2
21:06:41.60 +47:00:02.0
21:07:07.61 +47:46:43.8
21:08:24.96 +45:46:08.8
21:08:45.47 +47:24:13.5
21:13:14.74 +50:00:06.7
21:13:57.54 +48:56:54.7
21:15:09.21 +48:54:44.7
21:16:09.83 +47:29:32.1
21:18:58.01 +41:53:40.3
21:27:28.18 +43:54:55.2
21:28:29.72 +43:32:13.1
21:29:10.78 +47:17:36.4
21:31:29.60 +46:25:08.6
21:33:13.75 +44:27:07.8
21:33:24.18 +43:10:54.5
21:33:42.56 +47:16:17.8
21:35:38.85 +45:34:19.5
21:35:51.02 +45:24:27.0
21:37:05.51 +47:50:37.9
21:38:24.77 +47:22:55.9
21:38:31.43 +48:30:05.1
21:38:32.83 +49:46:26.9
21:39:17.08 +42:26:28.3
21:40:13.05 +45:27:16.2
21:41:01.96 +43:56:46.0
21:41:23.65 +47:01:13.7
21:41:57.34 +47:44:04.4
21:43:33.99 +49:08:56.2
21:43:55.61 +47:21:47.0
21:43:56.40 +47:21:45.0
21:45:01.52 +44:39:18.6
21:45:04.59 +47:54:05.0
21:47:07.04 +48:28:58.4
21:56:13.40 +47:40:53.0
21:57:15.79 +42:01:08.6
22:04:56.90 +47:35:01.3
21:01:42.99 +44:55:01.0
21:28:07.93 +48:30:09.1
21:11:17.54 +46:26:44.6
21:32:31.54 +49:26:55.0
21:31:04.12 +47:57:11.5
21:38:35.22 +47:44:28.6
####################################################
The observatory MPC code is 500
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461126.90532675 -observatory 500
22:47:08.97 -08:14:38.3 Mercury (0.6mag)
01:35:52.85 +09:18:56.0 Venus (-3.9mag)
23:21:46.61 -05:16:02.0 Mars (1.2mag)
07:05:55.18 +22:56:30.4 Jupiter (-2.2mag)
00:20:17.10 -00:07:16.6 Saturn (0.9mag)
03:43:57.58 +19:35:17.7 Uranus (5.8mag)
00:08:10.87 -00:32:17.6 Neptune (7.8mag)
20:32:32.72 -22:53:03.8 Pluto (14.5mag)
07:59:28.90 +24:07:34.4 Moon (-10.9mag)
-rw-r--r-- 1 apache apache 362 Mar 27 05:24 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461126.90532675:
07:05:49.45 +22:56:43.2 Io (5.6mag)
07:05:53.31 +22:56:30.6 Europa (5.8mag)
07:05:43.67 +22:56:45.4 Ganymede (5.2mag)
07:06:11.44 +22:56:09.4 Callisto (6.5mag)
07:09:52.68 +22:54:24.7 Himalia (15.2mag)
07:05:58.26 +22:56:22.6 Thebe (16.1mag)
07:09:36.03 +23:20:17.5 Elara (17.2mag)
07:03:28.47 +23:46:47.9 Pasiphae (17.3mag)
07:14:37.08 +22:52:03.5 Carme (18.4mag)
00:20:28.85 -00:07:13.7 Titan (8.8mag)
00:20:17.15 -00:07:01.3 Rhea (10.1mag)
00:20:38.41 -00:05:04.8 Iapetus (11.5mag)
00:20:18.70 -00:06:52.7 Hyperion (14.8mag)
00:22:07.65 +00:03:27.3 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Mar 27 05:24 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461126.90532675:
13:40:27.86 +01:52:45.4 JWST
18:10:06.37 +32:13:40.8 Chandra
08:56:27.58 -46:53:02.5 XMM-Newton
-rw-r--r-- 1 apache apache 96 Mar 27 05:24 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461126.90532675 -observatory 500
18:40:32.76 -27:45:09.4 14.0mag P/2010 H2 (Vales)
04:54:21.67 -70:40:22.5 17.5mag C/2014 UN271 (Bernardinelli-Bernstein)
05:29:15.51 +31:19:33.3 17.1mag C/2017 K2 (PANSTARRS)
17:30:28.44 +08:10:47.1 17.6mag C/2021 G2 (ATLAS)
23:03:59.14 +28:34:44.9 17.0mag C/2022 E2 (ATLAS)
04:07:14.30 +25:28:49.6 15.8mag C/2022 N2 (PANSTARRS)
09:01:29.85 +31:40:24.9 16.1mag C/2022 QE78 (ATLAS)
08:29:48.78 -02:23:16.6 17.2mag C/2022 R6 (PANSTARRS)
18:56:27.04 +16:50:40.6 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:45:31.54 -11:46:51.7 17.6mag P/2023 B1 (PANSTARRS)
09:19:26.93 -15:11:55.8 17.5mag C/2023 F3 (ATLAS)
21:30:54.26 +61:55:51.3 17.4mag C/2023 H5 (Lemmon)
19:31:11.07 -03:32:38.6 14.4mag C/2023 R1 (PANSTARRS)
21:40:52.83 +83:29:00.2 17.7mag C/2023 X2 (Lemmon)
06:14:00.19 +63:41:58.1 16.9mag C/2024 A1 (ATLAS)
04:25:39.28 +09:29:49.4 9.6mag C/2024 E1 (Wierzchos)
11:17:26.02 +03:58:55.4 18.0mag C/2024 G2 (ATLAS)
16:29:48.93 +03:11:00.5 17.4mag C/2024 G6 (ATLAS)
20:13:17.88 +10:15:40.0 14.8mag C/2024 J3 (ATLAS)
03:09:41.05 -25:32:48.3 16.4mag C/2024 T5 (ATLAS)
05:01:34.62 +50:37:37.9 17.6mag C/2025 J1 (Borisov)
14:54:41.68 +25:59:29.5 14.5mag C/2025 L1 (ATLAS)
02:56:45.70 -23:24:36.1 17.7mag C/2025 Q3 (ATLAS)
22:37:58.11 +19:26:33.7 11.6mag C/2025 R3 (PANSTARRS)
13:02:32.22 +01:44:26.6 17.6mag C/2025 Y1 (ATLAS)
01:50:59.37 -02:13:12.2 12.3mag C/2026 A1 (MAPS)
23:00:04.70 +32:51:43.6 13.9mag C/2026 B2 (Sun-Gao)
18:04:37.02 -10:37:52.6 13.0mag 10P/Tempel
15:22:40.90 +04:47:11.4 12.3mag 24P/Schaumasse
11:09:22.74 -02:13:59.5 15.6mag 29P/Schwassmann-Wachmann
17:49:43.18 -10:23:36.8 17.5mag 40P/Vaisala
10:42:06.62 -05:54:34.5 16.5mag 43P/Wolf-Harrington
01:18:37.77 +14:04:12.6 17.0mag 47P/Ashbrook-Jackson
06:37:40.63 +41:04:21.1 17.1mag 63P/Wild
23:03:05.78 -13:54:16.7 15.7mag 65P/Gunn
03:13:32.68 +13:56:27.9 15.9mag 76P/West-Kohoutek-Ikemura
00:23:03.44 +04:19:40.9 14.6mag 78P/Gehrels
22:00:32.51 -15:02:17.1 14.5mag 88P/Howell
01:17:10.31 +15:07:20.8 15.2mag 93P/Lovas
04:20:31.02 +31:06:33.2 16.4mag 123P/West-Hartley
08:10:31.05 +47:22:53.9 16.2mag 124P/Mrkos
02:03:38.79 +12:06:49.8 16.4mag 128P/Shoemaker-Holt
02:09:34.21 +11:56:02.0 17.4mag 131P/Mueller
23:48:55.72 +05:41:03.5 12.2mag 141P/Machholz
23:59:11.89 -02:18:23.8 12.3mag 141P-A/Machholz
22:55:49.72 -05:17:53.1 15.3mag 141P-D/Machholz
00:08:06.51 -11:09:21.0 15.4mag 162P/SidingSpring
10:35:19.53 +31:56:00.3 17.6mag 164P/Christensen
06:00:51.40 +24:41:19.8 17.6mag 198P/ODAS
15:24:29.28 -02:29:33.7 17.1mag 210P/Christensen
20:35:34.51 -16:07:53.5 17.2mag 218P/LINEAR
17:05:29.85 -16:05:31.7 16.2mag 235P/LINEAR
04:53:49.51 +32:48:05.8 16.4mag 240P/NEAT
07:31:09.25 -07:31:04.2 17.5mag 242P/Spahr
15:47:58.23 +05:35:00.3 17.6mag 391P/Kowalski
07:28:45.99 +21:12:18.6 17.6mag 450P/LONEOS
05:08:54.04 +46:12:30.1 17.3mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.8K Mar 27 05:24 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.87 -53:16:33.70 ASASSN-26cc 2026-03-20.08 3.93
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.90 -45:55:38.40 ASASSN-26bt 2026-03-19.05 16.24
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.45 +15:42:15.00 SN2026ehe 2026-03-12.11 -0.29
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
11:30:09.67 -47:26:43.70 ASASSN-26bn 2026-03-10.12 15.2
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.48 -37:49:32.80 ASASSN-26bk 2026-03-2.3 13.11
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.29 +19:58:46.30 ASASSN-26be 2026-02-25.56 14.95
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:35.79 -79:28:57.30 ASASSN-26bb 2026-02-24.37 16.2
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
04:55:50.66 -29:52:57.70 SN 2026dpg 2026-02-23.11 15.75
04:21:28.18 -53:22:54.40 AT2026drl 2026-02-21.03 17.31
11:50:37.32 +55:21:13.70 SN 2026dix 2026-02-21.43 16.39
16:21:19.69 -63:47:29.40 ASASSN-26az 2026-02-21.03 17.02
02:45:30.93 -54:17:43.10 SN 2026cju 2026-02-21.04 17.54
01:58:40.68 +47:34:50.10 ASASSN-26av 2026-02-21.09 15.97
18:35:53.01 -42:31:38.90 ASASSN-26aw 2026-02-21.12 15.89
11:40:18.88 -39:45:09.20 ASASSN-26ax 2026-02-21.08 15.73
02:26:23.52 -51:42:29.80 ASASSN-26ay 2026-02-21.04 13.93
08:46:07.66 +01:17:43.90 ASASSN-26ba 2026-02-20.23 15.43
14:15:47.69 -48:05:16.40 SN2026dez 2026-02-19.19 15.93
17:25:53.90 -23:28:31.50 ASASSN-26au 2026-02-18.33 15.82
16:07:59.09 -24:00:10.00 SN2026cmv 2026-02-17.28 16.19
18:15:01.25 -37:43:36.70 ASASSN-26at 2026-02-16.36 15.94
13:01:07.08 -11:25:16.30 AT2026bzh 2026-02-12.45 17.3
10:56:29.81 -07:07:25.30 SN 2026bre 2026-02-12.16 17.15
08:55:43.51 -53:26:11.50 ASASSN-26as 2026-02-12.2 16.54
06:33:50.98 -41:46:25.10 ASASSN-26ar 2026-02-12.04 16.42
12:15:22.43 +23:59:39.60 SN2026bzg 2026-02-11.27 16.32
08:01:10.95 -03:43:14.30 AT2026coj 2026-02-9.25 13.73
12:44:00.18 -57:03:46.80 ASASSN-26aq 2026-02-9.18 16
06:26:33.34 -54:06:39.90 AT2026cih 2026-02-8.06 17.26
23:08:59.40 -88:59:11.60 SN 2026bsu 2026-02-8.03 16.02
01:04:14.94 -62:31:02.30 SN 2026azk 2026-02-8.04 16.41
08:44:55.41 +64:55:09.90 SN 2026anq 2026-02-7.16 17.62
12:37:42.99 +33:26:05.40 SN 2026bnm 2026-02-7.29 16.74
00:12:55.45 +33:21:25.90 SN2026cbh 2026-02-7.09 16.33
08:02:12.64 -04:14:20.90 SN 2026auh 2026-02-7.11 16.64
18:03:52.67 -31:27:26.00 TCP J18035290-3127298 2026-02-7.37 15.76
12:18:03.59 +50:27:10.20 SN 2026bjz 2026-02-7.25 16.48
07:51:51.12 +55:05:27.60 SN 2026ail 2026-02-6.21 16.85
08:10:56.38 +36:49:42.80 AT2026bsa 2026-02-6.29 17.47
04:43:45.47 -15:49:01.00 SN2026azr 2026-02-5.24 16.96
06:14:48.48 -34:20:08.90 ASASSN-26ap 2026-02-5.2 13.77
02:42:33.90 -27:21:02.60 SN 2026aip 2026-02-4.09 15.85
00:43:12.26 +38:35:47.90 AT2026brt 2026-02-3.12 14.92
14:34:27.21 +21:56:59.90 SN2026atb 2026-01-29.32 15.59
13:12:04.11 -60:56:12.40 ASASSN-26ao 2026-01-28.35 15.61
13:00:36.49 -06:28:26.00 SN2026azd 2026-01-28.23 15.69
10:33:50.27 -31:00:53.40 SN 2026ayz 2026-01-25.11 15.3
-rw-r--r-- 1 apache apache 5.8K Mar 27 05:24 asassn_transients_list.txt
############################################################
Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
15:33:45.28 -22:11:07.3 TCP J15334528-2211073 2026-01-16.8451 14.9mag
22:34:01.26 +39:53:32.8 TCP J22340126+3953328 2026-01-17.5738 16.79Cmag
00:42:52.36 +41:16:13.3 PNV J00425236+4116133 2026-01-18.5502 17.41Cmag
06:57:11.19 -17:24:43.9 TCP J06571119-1724439 2026-01-18.5375 14.2mag
00:42:52.23 +41:01:44.7 PNV J00425223+4101447 2026-01-19.5505 18.74Cmag
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
-rw-r--r-- 1 apache apache 187K Mar 27 05:24 tocp_transients_list.txt