This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK
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
NSVS J2212515+391002,2461121.9474,10.85,0.05,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 J2212515+391002 20260322.4474 10.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:12:51.19 +39:09:59.7 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.9474,12.73,0.05,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
target 20260322.4474 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:32:45.89 +37:06:35.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.4474 2461121.9474 12.54 21:54:20.75 +40:56:10.6
90.49459 -10.52325 galactic Cyg Second-epoch detections are separated by 3.3" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:54:20.75 +40:56:10.6 (user input) | T | P | (position from user input) J-Ks=0.733+/-0.033 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.9474,12.54,0.05,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
target 20260322.4474 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:54:20.75 +40:56:10.6 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.4474 2461121.9474 12.21 21:19:27.97 +36:07:29.4
82.09826 -9.43196 galactic Cyg Second-epoch detections are separated by 6.8" 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 J319.8655+36.1270 | 21:19:27.97 +36:07:29.4 (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 J319.8655+36.1270,2461121.9474,12.21,0.05,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 J319.8655+36.1270 20260322.4474 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:19:27.97 +36:07:29.4 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.4474 2461121.9474 12.25 21:25:28.13 +34:19:08.3
81.65477 -11.57055 galactic Cyg Second-epoch detections are separated by 0.8" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:25:28.13 +34:19:08.3 (user input) | T | P | (position from user input) J-Ks=0.760+/-0.025 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.9474,12.25,0.05,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
target 20260322.4474 12.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:25:28.13 +34:19:08.3 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.4474 2461121.9474 12.43 21:44:37.49 +38:02:16.8
87.12796 -11.52116 galactic Cyg Second-epoch detections are separated by 1.9" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:44:37.49 +38:02:16.8 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.9474,12.43,0.05,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
target 20260322.4474 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:44:37.49 +38:02:16.8 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_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 1964864735256226432,2461121.9474,11.97,0.05,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 1964864735256226432 20260322.4474 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:20:00.27 +38:24:38.4 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.4474 2461121.9474 11.99 21:31:04.47 +40:43:44.2
87.01095 -7.76898 galactic Cyg Second-epoch detections are separated by 2.2" and 4.9 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 J322.7701+40.7254 | 21:31:04.47 +40:43:44.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.670+/-0.030 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J322.7701+40.7254,2461121.9474,11.99,0.05,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 J322.7701+40.7254 20260322.4474 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:31:04.47 +40:43:44.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.9474,11.94,0.05,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
target 20260322.4474 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:36:13.70 +40:51:40.8 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.4474 2461121.9474 11.80 21:19:40.96 +35:26:24.6
81.62854 -9.93823 galactic Cyg Second-epoch detections are separated by 6.0" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J319.9241+35.4340 | 21:19:40.96 +35:26:24.6 (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 J319.9241+35.4340,2461121.9474,11.80,0.05,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 J319.9241+35.4340 20260322.4474 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:19:40.96 +35:26:24.6 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.4474 2461121.9474 11.82 21:27:41.77 +38:45:47.0
85.15984 -8.73353 galactic Cyg Second-epoch detections are separated by 2.5" 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 J321.9265+38.7675 | 21:27:41.77 +38:45:47.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.638+/-0.035 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J321.9265+38.7675,2461121.9474,11.82,0.05,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 J321.9265+38.7675 20260322.4474 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:27:41.77 +38:45:47.0 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.9474,11.82,0.05,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
target 20260322.4474 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:16:20.03 +38:24:01.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.4474 2461121.9474 11.94 21:48:12.45 +41:41:13.0
90.08186 -9.20920 galactic Cyg Second-epoch detections are separated by 0.3" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1960503900338500992 | 21:48:14.24 +41:40:60.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.489+/-0.045 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1960503900338500992,2461121.9474,11.94,0.05,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 1960503900338500992 20260322.4474 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:48:12.45 +41:41:13.0 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_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 1964854770931615872,2461121.9474,11.77,0.05,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 1964854770931615872 20260322.4474 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:18:47.25 +38:10:23.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.4474 2461121.9474 11.69 21:23:43.93 +35:58:31.6
82.60044 -10.15372 galactic Cyg Second-epoch detections are separated by 1.9" 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 | target | 21:23:43.93 +35:58:31.6 (user input) | T | P | (position from user input) J-Ks=0.340+/-0.030 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.9474,11.69,0.05,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
target 20260322.4474 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:23:43.93 +35:58:31.6 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.4474 2461121.9474 11.62 21:28:46.84 +42:05:19.7
87.64440 -6.48871 galactic Cyg Second-epoch detections are separated by 2.1" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:28:46.84 +42:05:19.7 (user input) | T | P | (position from user input) J-Ks=0.784+/-0.027 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.9474,11.62,0.05,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
target 20260322.4474 11.62CV 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:28:46.84 +42:05:19.7 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.4474 2461121.9474 11.50 21:27:24.06 +33:39:58.6
81.46996 -12.31467 galactic Cyg Second-epoch detections are separated by 3.8" 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 | Gaia DR3 1854304305596960256 | 21:27:21.99 +33:40:12.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.297+/-0.028 (F)
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 1854304305596960256,2461121.9474,11.50,0.05,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 1854304305596960256 20260322.4474 11.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:27:24.06 +33:39:58.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.4474 2461121.9474 11.41 21:19:57.91 +39:52:34.6
84.88672 -6.88923 galactic Cyg Second-epoch detections are separated by 2.9" 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 J319.9852+39.8763 | 21:19:57.91 +39:52:34.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.763+/-0.231 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J319.9852+39.8763,2461121.9474,11.41,0.05,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
ATO J319.9852+39.8763 20260322.4474 11.41CV 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:19:57.91 +39:52:34.6 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_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 J2141045+415639,2461121.9474,11.35,0.05,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 J2141045+415639 20260322.4474 11.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:41:05.58 +41:56:41.8 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.4474 2461121.9474 11.35 21:22:57.05 +34:21:07.1
81.30727 -11.17656 galactic Cyg Second-epoch detections are separated by 0.8" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1855344649753169280 | 21:22:54.85 +34:21:08.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1855344649753169280,2461121.9474,11.35,0.05,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 1855344649753169280 20260322.4474 11.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:22:57.05 +34:21:07.1 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_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 1964745159067548800,2461121.9474,11.17,0.05,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 1964745159067548800 20260322.4474 11.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:18:16.67 +37:55:33.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.4474 2461121.9474 10.96 21:46:27.06 +42:00:04.1
90.03601 -8.75789 galactic Cyg Second-epoch detections are separated by 2.0" 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 | target | 21:46:27.06 +42:00:04.1 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.741+/-0.034 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.9474,10.96,0.05,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
target 20260322.4474 10.96CV 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:46:27.06 +42:00:04.1 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.4474 2461121.9474 10.89 22:14:06.05 +39:37:06.3
92.74055 -13.85645 galactic Lac Second-epoch detections are separated by 1.1" 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 J333.5265+39.6221 | 22:14:04.48 +39:37:10.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.301+/-0.031 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J333.5265+39.6221,2461121.9474,10.89,0.05,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 J333.5265+39.6221 20260322.4474 10.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:14:06.05 +39:37:06.3 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.4474 2461121.9474 9.81 21:27:38.48 +37:49:02.3
84.48180 -9.40155 galactic Cyg Second-epoch detections are separated by 0.5" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1964212205163543680 | 21:27:37.21 +37:48:57.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1964212205163543680,2461121.9474,9.81,0.05,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
Gaia DR3 1964212205163543680 20260322.4474 9.81CV 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:27:38.48 +37:49:02.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.4474 2461121.9474 10.54 21:47:57.29 +36:35:34.4
86.66426 -13.04477 galactic Cyg Second-epoch detections are separated by 0.8" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1952454543207886464 | 21:47:57.30 +36:35:34.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.751+/-0.030 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1952454543207886464,2461121.9474,10.54,0.05,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 1952454543207886464 20260322.4474 10.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:47:57.29 +36:35:34.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.4474 2461121.9474 10.65 21:42:55.13 +41:10:18.7
88.98109 -8.95135 galactic Cyg Second-epoch detections are separated by 2.3" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1954518120374734464 | 21:42:55.04 +41:10:18.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.059+/-0.044 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1954518120374734464,2461121.9474,10.65,0.05,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
Gaia DR3 1954518120374734464 20260322.4474 10.65CV 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:42:55.13 +41:10:18.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_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
V1907 Cyg,2461121.9474,10.76,0.05,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
V1907 Cyg 20260322.4474 10.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:31:14.77 +39:26:59.5 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_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 1952708225458525824,2461121.9474,10.82,0.05,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 1952708225458525824 20260322.4474 10.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:42:50.23 +37:29:34.1 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.4474 2461121.9474 11.19 21:52:09.50 +38:58:10.4
88.88938 -11.77361 galactic Cyg Second-epoch detections are separated by 0.8" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:52:09.50 +38:58:10.4 (user input) | T | P | (position from user input) J-Ks=0.770+/-0.029 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.9474,11.19,0.05,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
target 20260322.4474 11.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:52:09.50 +38:58:10.4 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_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
V1338 Cyg,2461121.9474,11.09,0.05,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
V1338 Cyg 20260322.4474 11.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:35:04.73 +40:51:23.3 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.4474 2461121.9474 11.34 22:13:14.49 +41:47:44.0
93.90034 -11.98864 galactic Lac Second-epoch detections are separated by 0.7" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J333.2961+41.7989 | 22:13:14.49 +41:47:44.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.941+/-0.026 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J333.2961+41.7989,2461121.9474,11.34,0.05,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 J333.2961+41.7989 20260322.4474 11.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:13:14.49 +41:47:44.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.4474 2461121.9474 11.45 22:08:10.05 +37:08:03.6
90.25360 -15.17027 galactic Lac Second-epoch detections are separated by 2.2" 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 | ASASSN-V J220810.13+370722.7 | 22:08:10.14 +37:07:22.6 (Gaia DR3) | L (local) | (local) | Gaia3var=VARIABLE SpType: M7 1986ApJ...301..927S StM 551
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J220810.13+370722.7,2461121.9474,11.45,0.05,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
ASASSN-V J220810.13+370722.7 20260322.4474 11.45CV 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:08:10.05 +37:08:03.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.4474 2461121.9474 11.30 21:33:36.31 +38:32:49.9
85.85130 -9.68826 galactic Cyg Second-epoch detections are separated by 2.3" 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 | target | 21:33:36.31 +38:32:49.9 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.285+/-0.031 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.9474,11.30,0.05,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
target 20260322.4474 11.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:33:36.31 +38:32:49.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.4474 2461121.9474 11.53 22:07:50.33 +40:07:28.7
92.04956 -12.73949 galactic Lac Second-epoch detections are separated by 0.8" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J331.9519+40.1216 | 22:07:50.33 +40:07:28.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.493+/-0.031 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J331.9519+40.1216,2461121.9474,11.53,0.05,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
ATO J331.9519+40.1216 20260322.4474 11.53CV 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:07:50.33 +40:07:28.7 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.4474 2461121.9474 11.40 21:31:28.50 +35:34:31.7
83.44977 -11.54313 galactic Cyg Second-epoch detections are separated by 1.8" 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 J322.8685+35.5755 | 21:31:29.78 +35:35:00.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.195+/-0.028 (F)
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 J322.8685+35.5755,2461121.9474,11.40,0.05,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 J322.8685+35.5755 20260322.4474 11.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:31:28.50 +35:34:31.7 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.4474 2461121.9474 11.52 21:55:05.22 +34:46:32.0
86.58441 -15.36720 galactic Peg Second-epoch detections are separated by 1.1" 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 | target | 21:55:05.22 +34:46:32.0 (user input) | T | P | (position from user input) J-Ks=0.439+/-0.033 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.9474,11.52,0.05,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
target 20260322.4474 11.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:55:05.22 +34:46:32.0 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_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 1952713070181680896,2461121.9474,11.56,0.05,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
Gaia DR3 1952713070181680896 20260322.4474 11.56CV 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:42:56.20 +37:35:03.8 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.4474 2461121.9474 11.64 22:11:22.97 +39:44:16.4
92.37584 -13.45374 galactic Lac Second-epoch detections are separated by 1.4" 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 | target | 22:11:22.97 +39:44:16.4 (user input) | T | P | (position from user input) J-Ks=0.721+/-0.028 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.9474,11.64,0.05,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
target 20260322.4474 11.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:11:22.97 +39:44:16.4 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.4474 2461121.9474 11.32 21:18:39.97 +39:14:37.5
84.25415 -7.15114 galactic Cyg Second-epoch detections are separated by 2.0" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1965155379979232000 | 21:18:40.87 +39:14:20.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.314+/-0.033 (F)
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 1965155379979232000,2461121.9474,11.32,0.05,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 1965155379979232000 20260322.4474 11.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:18:39.97 +39:14:37.5 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.4474 2461121.9474 11.47 21:42:50.12 +38:10:46.0
86.95487 -11.18187 galactic Cyg Second-epoch detections are separated by 2.1" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.6987+38.1778 | 21:42:50.12 +38:10:46.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.374+/-0.041 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.6987+38.1778,2461121.9474,11.47,0.05,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
ATO J325.6987+38.1778 20260322.4474 11.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:42:50.12 +38:10:46.0 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.4474 2461121.9474 11.57 21:35:30.55 +34:46:53.3
83.49641 -12.68675 galactic Cyg Second-epoch detections are separated by 1.7" 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 | target | 21:35:30.55 +34:46:53.3 (user input) | T | P | (position from user input) J-Ks=0.777+/-0.029 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.9474,11.57,0.05,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
target 20260322.4474 11.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:35:30.55 +34:46:53.3 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.4474 2461121.9474 11.73 22:00:54.54 +41:16:15.5
91.69126 -11.03182 galactic Lac Second-epoch detections are separated by 3.3" 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 | target | 22:00:54.54 +41:16:15.5 (user input) | T | P | (position from user input) J-Ks=0.301+/-0.044 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.9474,11.73,0.05,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
target 20260322.4474 11.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:00:54.54 +41:16:15.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.4474 2461121.9474 11.78 22:02:40.16 +38:06:49.0
89.97780 -13.73055 galactic Lac Second-epoch detections are separated by 1.5" 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 J330.6734+38.1123 | 22:02:40.16 +38:06:49.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G1 (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 J330.6734+38.1123,2461121.9474,11.78,0.05,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 J330.6734+38.1123 20260322.4474 11.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:02:40.16 +38:06:49.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_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 1955341212206396160,2461121.9474,11.94,0.05,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 1955341212206396160 20260322.4474 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:14:09.52 +38:28:30.5 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.4474 2461121.9474 11.81 21:23:19.17 +35:13:34.5
81.99771 -10.61939 galactic Cyg Second-epoch detections are separated by 3.5" 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 J320.8355+35.2221 | 21:23:19.17 +35:13:34.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J320.8355+35.2221,2461121.9474,11.81,0.05,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 J320.8355+35.2221 20260322.4474 11.81CV 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:23:19.17 +35:13:34.5 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.4474 2461121.9474 11.85 21:44:49.77 +36:56:56.3
86.42239 -12.36445 galactic Cyg Second-epoch detections are separated by 1.6" 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 | target | 21:44:49.77 +36:56:56.3 (user input) | T | P | (position from user input) J-Ks=0.402+/-0.045 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.9474,11.85,0.05,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
target 20260322.4474 11.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:44:49.77 +36:56:56.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.4474 2461121.9474 11.79 21:49:54.63 +34:54:45.1
85.83935 -14.57426 galactic Peg Second-epoch detections are separated by 1.3" 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 | target | 21:49:54.63 +34:54:45.1 (user input) | T | P | (position from user input) J-Ks=0.280+/-0.040 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.9474,11.79,0.05,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
target 20260322.4474 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:49:54.63 +34:54:45.1 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.4474 2461121.9474 11.77 21:41:14.03 +41:15:46.6
88.80190 -8.67324 galactic Cyg Second-epoch detections are separated by 4.4" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.3088+41.2622 | 21:41:14.03 +41:15:46.6 (user input) | MSINE (ATLAS) | (ATLAS) | (position from user input) SpType: G2 (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 J325.3088+41.2622,2461121.9474,11.77,0.05,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 J325.3088+41.2622 20260322.4474 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:41:14.03 +41:15:46.6 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.4474 2461121.9474 11.85 21:59:27.32 +38:47:14.0
89.89827 -12.81201 galactic Lac Second-epoch detections are separated by 4.1" 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 | target | 21:59:27.32 +38:47:14.0 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.9474,11.85,0.05,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
target 20260322.4474 11.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:59:27.32 +38:47:14.0 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.4474 2461121.9474 11.84 22:21:21.24 +41:17:36.1
94.88801 -13.26430 galactic Lac Second-epoch detections are separated by 2.2" 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 J335.3499+41.2971 | 22:21:21.24 +41:17:36.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J335.3499+41.2971,2461121.9474,11.84,0.05,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 J335.3499+41.2971 20260322.4474 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:21:21.24 +41:17:36.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.4474 2461121.9474 11.90 22:03:59.96 +39:46:43.0
91.23409 -12.57185 galactic Lac Second-epoch detections are separated by 1.7" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:03:59.96 +39:46:43.0 (user input) | T | P | (position from user input) J-Ks=0.937+/-0.032 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.9474,11.90,0.05,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
target 20260322.4474 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:03:59.96 +39:46:43.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.4474 2461121.9474 11.90 22:13:05.33 +41:48:42.2
93.88622 -11.95897 galactic Lac Second-epoch detections are separated by 1.2" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:13:05.33 +41:48:42.2 (user input) | T | P | (position from user input) J-Ks=0.719+/-0.028 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.9474,11.90,0.05,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
target 20260322.4474 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:13:05.33 +41:48:42.2 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.4474 2461121.9474 11.88 21:57:20.66 +40:56:59.8
90.95177 -10.86821 galactic Cyg Second-epoch detections are separated by 2.1" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.3425+40.9483 | 21:57:22.82 +40:57:15.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.451+/-0.035 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.3425+40.9483,2461121.9474,11.88,0.05,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
ATO J329.3425+40.9483 20260322.4474 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:57:20.66 +40:56:59.8 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.4474 2461121.9474 11.96 22:13:03.51 +38:28:18.7
91.88048 -14.66931 galactic Lac Second-epoch detections are separated by 3.3" 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 | target | 22:13:03.51 +38:28:18.7 (user input) | T | P | (position from user input) J-Ks=0.384+/-0.030 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.9474,11.96,0.05,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
target 20260322.4474 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:13:03.51 +38:28:18.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.4474 2461121.9474 12.05 22:13:03.62 +38:27:57.2
91.87716 -14.67436 galactic Lac Second-epoch detections are separated by 1.1" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:13:03.62 +38:27:57.2 (user input) | T | P | (position from user input) J-Ks=0.456+/-0.035 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.9474,12.05,0.05,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
target 20260322.4474 12.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:13:03.62 +38:27:57.2 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.4474 2461121.9474 12.02 22:02:27.76 +42:04:06.0
92.42131 -10.57825 galactic Lac Second-epoch detections are separated by 4.0" 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 J330.6159+42.0668 | 22:02:27.76 +42:04:06.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J330.6159+42.0668,2461121.9474,12.02,0.05,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
ATO J330.6159+42.0668 20260322.4474 12.02CV 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:02:27.76 +42:04:06.0 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.4474 2461121.9474 12.02 21:58:15.43 +41:40:34.9
91.54824 -10.40626 galactic Lac Second-epoch detections are separated by 0.3" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:58:15.43 +41:40:34.9 (user input) | T | P | (position from user input) J-Ks=0.255+/-0.040 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.9474,12.02,0.05,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
target 20260322.4474 12.02CV 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:58:15.43 +41:40:34.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.4474 2461121.9474 12.03 22:06:31.82 +34:33:33.6
88.34988 -17.01291 galactic Peg Second-epoch detections are separated by 0.5" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:06:31.82 +34:33:33.6 (user input) | T | P | (position from user input) J-Ks=0.631+/-0.028 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.9474,12.03,0.05,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
target 20260322.4474 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:06:31.82 +34:33:33.6 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.4474 2461121.9474 12.16 21:59:28.72 +37:59:48.7
89.39621 -13.43300 galactic Lac Second-epoch detections are separated by 0.6" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.8746+37.9877 | 21:59:28.72 +37:59:48.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.437+/-0.036 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.8746+37.9877,2461121.9474,12.16,0.05,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 J329.8746+37.9877 20260322.4474 12.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:59:28.72 +37:59:48.7 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.4474 2461121.9474 12.03 22:15:17.48 +39:47:55.2
93.04031 -13.84212 galactic Lac Second-epoch detections are separated by 1.0" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:15:17.48 +39:47:55.2 (user input) | T | P | (position from user input) J-Ks=0.376+/-0.030 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.9474,12.03,0.05,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
target 20260322.4474 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:15:17.48 +39:47:55.2 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_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 1949071109713094272,2461121.9474,12.05,0.05,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 1949071109713094272 20260322.4474 12.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:50:11.33 +35:33:10.6 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_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 1956026134933788544,2461121.9474,12.14,0.05,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 1956026134933788544 20260322.4474 12.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:00:00.02 +38:42:25.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.9474,12.11,0.05,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
target 20260322.4474 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:42:24.37 +38:38:05.5 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.4474 2461121.9474 12.15 22:07:43.23 +37:37:05.9
90.48222 -14.73059 galactic Lac Second-epoch detections are separated by 2.1" 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 J331.9384+37.6117 | 22:07:43.23 +37:37:05.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.166+/-0.036 (F)
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 J331.9384+37.6117,2461121.9474,12.15,0.05,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 J331.9384+37.6117 20260322.4474 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:07:43.23 +37:37:05.9 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.4474 2461121.9474 12.13 22:04:36.75 +38:54:17.0
90.78497 -13.33747 galactic Lac Second-epoch detections are separated by 1.6" 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 | Gaia DR3 1955939827569816448 | 22:04:34.49 +38:53:59.0 (Gaia DR3) | DSCT/GDOR (local) | (local) | Gaia3var=VARIABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1955939827569816448,2461121.9474,12.13,0.05,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
Gaia DR3 1955939827569816448 20260322.4474 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:04:36.75 +38:54:17.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.4474 2461121.9474 12.15 22:03:22.55 +37:41:21.5
89.82226 -14.15087 galactic Lac Second-epoch detections are separated by 3.5" 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 J330.8446+37.6887 | 22:03:22.55 +37:41:21.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J330.8446+37.6887,2461121.9474,12.15,0.05,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 J330.8446+37.6887 20260322.4474 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:03:22.55 +37:41:21.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_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
V1616 Cyg,2461121.9474,12.18,0.05,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
V1616 Cyg 20260322.4474 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:41:09.79 +36:39:10.0 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.4474 2461121.9474 12.13 21:52:31.15 +41:28:59.4
90.57681 -9.88249 galactic Cyg Second-epoch detections are separated by 4.3" 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 | Gaia DR3 1960357802729664512 | 21:52:34.39 +41:28:42.5 (Gaia DR3) | ROT (local) | (local) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1960357802729664512,2461121.9474,12.13,0.05,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
Gaia DR3 1960357802729664512 20260322.4474 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:52:31.15 +41:28:59.4 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.9474,12.11,0.05,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
target 20260322.4474 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:06:04.04 +39:59:13.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.9474,12.34,0.05,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
target 20260322.4474 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:50:34.13 +37:11:05.5 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.4474 2461121.9474 12.26 21:56:00.49 +37:10:59.3
88.31998 -13.63282 galactic Cyg Second-epoch detections are separated by 1.0" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J328.9918+37.1927 | 21:56:00.49 +37:10:59.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.478+/-0.033 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J328.9918+37.1927,2461121.9474,12.26,0.05,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 J328.9918+37.1927 20260322.4474 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:56:00.49 +37:10:59.3 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.9474,12.22,0.05,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
target 20260322.4474 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:46:36.53 +37:39:36.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.4474 2461121.9474 12.13 21:31:28.73 +34:33:30.5
82.72624 -12.27326 galactic Cyg Second-epoch detections are separated by 2.3" 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 | target | 21:31:28.73 +34:33:30.5 (user input) | T | P | (position from user input) J-Ks=0.303+/-0.026 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.9474,12.13,0.05,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
target 20260322.4474 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:31:28.73 +34:33:30.5 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.4474 2461121.9474 12.28 21:37:55.36 +36:14:23.5
84.88440 -11.95919 galactic Cyg Second-epoch detections are separated by 0.6" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J324.4847+36.2365 | 21:37:55.36 +36:14:23.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J324.4847+36.2365,2461121.9474,12.28,0.05,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 J324.4847+36.2365 20260322.4474 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:37:55.36 +36:14:23.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.4474 2461121.9474 12.38 21:41:50.91 +35:55:33.8
85.26575 -12.72654 galactic Cyg Second-epoch detections are separated by 0.7" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.4608+35.9170 | 21:41:50.91 +35:55:33.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.355+/-0.038 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.4608+35.9170,2461121.9474,12.38,0.05,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
ATO J325.4608+35.9170 20260322.4474 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:41:50.91 +35:55:33.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_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 1960422738334188544,2461121.9474,12.41,0.05,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
Gaia DR3 1960422738334188544 20260322.4474 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:51:42.39 +41:44:43.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.4474 2461121.9474 12.49 21:43:03.21 +37:32:32.8
86.55521 -11.68603 galactic Cyg Second-epoch detections are separated by 2.1" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:43:03.21 +37:32:32.8 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.406+/-0.038 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.9474,12.49,0.05,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
target 20260322.4474 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:43:03.21 +37:32:32.8 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.4474 2461121.9474 12.78 21:50:24.65 +34:50:30.3
85.87173 -14.69492 galactic Peg Second-epoch detections are separated by 4.1" 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 | target | 21:50:24.65 +34:50:30.3 (user input) | T | P | (position from user input) J-Ks=0.319+/-0.045 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.9474,12.78,0.05,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
target 20260322.4474 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:50:24.65 +34:50:30.3 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.4474 2461121.9474 12.69 21:50:58.68 +36:44:37.8
87.23748 -13.32550 galactic Cyg Second-epoch detections are separated by 2.2" 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 | target | 21:50:58.68 +36:44:37.8 (user input) | T | P | (position from user input) J-Ks=0.402+/-0.041 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.9474,12.69,0.05,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
target 20260322.4474 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:50:58.68 +36:44:37.8 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.4474 2461121.9474 12.68 21:28:20.89 +36:09:01.6
83.39726 -10.68916 galactic Cyg Second-epoch detections are separated by 1.9" 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 J322.0938+36.1463 | 21:28:20.89 +36:09:01.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.753+/-0.031 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J322.0938+36.1463,2461121.9474,12.68,0.05,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 J322.0938+36.1463 20260322.4474 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:28:20.89 +36:09:01.6 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_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 1951490619409869568,2461121.9474,12.82,0.05,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 1951490619409869568 20260322.4474 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:24:37.60 +35:22:22.9 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.4474 2461121.9474 12.88 21:58:42.44 +41:08:27.9
91.27773 -10.87845 galactic Lac Second-epoch detections are separated by 2.3" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 1959914665183885568 | 21:58:41.59 +41:07:54.5 (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) J-Ks=0.290+/-0.049 (F)
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 1959914665183885568,2461121.9474,12.88,0.05,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
Large-amplitude variable Gaia DR2 1959914665183885568 20260322.4474 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:58:42.44 +41:08:27.9 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_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
IT Peg,2461121.9474,10.67,0.05,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
IT Peg 20260322.4474 10.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:03:42.55 +35:43:47.3 ;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-07-Q2b1x1_2025-12-22_20-20-53_20_00sec_-14_90C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20_00sec_-14_90C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20_00sec_-14_90C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20_00sec_-14_90C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_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
WW Peg,2461121.9474,10.58,0.05,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
WW Peg 20260322.4474 10.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:56:38.07 +36:20:35.0 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.4474 2461121.9474 11.71 21:50:52.42 +39:37:43.0
89.12653 -11.10871 galactic Cyg Second-epoch detections are separated by 1.0" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J327.7283+39.6224 | 21:50:52.42 +39:37:43.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.697+/-0.028 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J327.7283+39.6224,2461121.9474,11.71,0.05,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 J327.7283+39.6224 20260322.4474 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:50:52.42 +39:37:43.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20_00sec_-14_90C_LIGHT_0381_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20_00sec_-14_90C_LIGHT_0380_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: 2461032.59720919 23.12.2025 02:19:48.874 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits
First image: 2461032.59720919 23.12.2025 02:19:48.874 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits
Last image: 2461121.94770435 22.03.2026 10:44:31.656 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 10
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.77
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: 6 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): 24432
Objects passed selection criteria: 24356
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 19865.8
Average stars matched: 18545 (93.3516 %)
Memory usage VmPeak: 128452 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 Sun Mar 22 08:02:56 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: 2461032.59720919 23.12.2025 02:19:48.874 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits
First image: 2461032.59720919 23.12.2025 02:19:48.874 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits
Last image: 2461121.94770435 22.03.2026 10:44:31.656 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 131
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.43
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: 85 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): 173663
Objects passed selection criteria: 173221
Measurements per detected object (mean, median, min, max): 3.1 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 142680
Average stars matched: 132544 (92.8955 %)
Memory usage VmPeak: 2186124 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 Sun Mar 22 08:06:03 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits
SExtractor catalog cache: saved Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits.cat to cache
SExtractor catalog cache: saved Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.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: 2461121.94714414
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits exists and is non-empty
Saving wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits to local_wcs_cache/
'wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits' -> 'local_wcs_cache/wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits'
wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits exists and is non-empty
Saving wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits to local_wcs_cache/
'wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits' -> 'local_wcs_cache/wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits'
wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits exists and is non-empty
Saving wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits to local_wcs_cache/
'wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits' -> 'local_wcs_cache/wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits'
wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits exists and is non-empty
Saving wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits to local_wcs_cache/
'wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits' -> 'local_wcs_cache/wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits'
The image scale is 5.78"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.7"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 21:48:48.775 +38:01:54.18
Second-epoch image center 21:49:09.074 +37:57:50.35
Angular distance between the image centers 0.10 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 21:48:48.775 +38:01:54.18
Second-epoch image center 21:49:08.467 +37:58:16.06
Angular distance between the image centers 0.09 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 21:49:09.074 +37:57:50.35
Second-epoch second image center 21:49:08.467 +37:58:16.06
Angular distance between the image centers 0.00741 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits &> /tmp/tmp.nozwbczZdu
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits &> /tmp/tmp.llcRBh7K6s
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits &> /tmp/tmp.E4p0X4SN3R
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits &> /tmp/tmp.kauV7jFWr1
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits and wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits and wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits.cat
Found non-empty wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits and wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits.cat
The reference image (wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits) and catalog (wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits.cat) found
'wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.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 53 out of 28648 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.917418
a=0.000000 b=1.000000 c=22.917418
From vast_summary.log: estimated ref. image limiting mag.: -7.77
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.15
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.15
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 9 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits
2.2 pix Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
2.6 pix fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits
2.6 pix fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits
Limiting magnitude estimates:
15.1 mag. Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits
15.1 mag. Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
14.6 mag. fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits
14.6 mag. fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits
All-image limiting magnitude estimate: 14.6 (SNR ) 11.9 (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.nozwbczZdu (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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.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_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits' -> 'wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits
WCS_IMAGE_NAME=wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits
WCS-calibrated image found: wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits
Checking if the catalog wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits.cat corresponding to the image wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits alredy exist and is non-empty...
Catalog wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits.cat corresponding to the image wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits
WCS catalog name: wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2966, passed=28648
Got 28648 stars (including 25648 good ones) from the SExtractor catalog wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits.cat
util/solve_plate_with_UCAC5 got 28648 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 923.2'
Seting catalog search parameters based on the expected field of view 923.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012822 (46.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010258 (36.9 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 373 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 4.60"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 5.34"
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 467 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 5.39"
Estimated accuracy of the plate solution: 6.34"
Excluding outliers - 409 stars left (next iteration limit 332)
The image catalog is written to wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits -region wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.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.llcRBh7K6s (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-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.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_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits 572.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.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-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.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-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits' -> 'wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
WCS_IMAGE_NAME=wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
WCS-calibrated image found: wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
Checking if the catalog wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat corresponding to the image wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits alredy exist and is non-empty...
Catalog wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat corresponding to the image wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
WCS catalog name: wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2960, passed=28429
Got 28429 stars (including 25433 good ones) from the SExtractor catalog wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat
util/solve_plate_with_UCAC5 got 28429 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 932.3'
Seting catalog search parameters based on the expected field of view 932.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012949 (46.6 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010359 (37.3 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 424 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 3.43"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 3.46"
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 495 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 3.41"
Estimated accuracy of the plate solution: 2.48"
Excluding outliers - 452 stars left (next iteration limit 410)
The image catalog is written to wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits -region wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.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.E4p0X4SN3R (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_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.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_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits
WCS-calibrated image found: wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits
Checking if the catalog wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits
WCS catalog name: wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1439, passed=19873
Got 19873 stars (including 18417 good ones) from the SExtractor catalog wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits.cat
util/solve_plate_with_UCAC5 got 19873 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.1'
Seting catalog search parameters based on the expected field of view 939.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013043 (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 0.010434 (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 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: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.58"
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: 0.58"
Estimated accuracy of the plate solution: 0.65"
Excluding outliers - 959 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits -region wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.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.kauV7jFWr1 (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_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.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_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits
WCS-calibrated image found: wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits
Checking if the catalog wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits
WCS catalog name: wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1380, passed=19930
Got 19930 stars (including 18531 good ones) from the SExtractor catalog wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits.cat
util/solve_plate_with_UCAC5 got 19930 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.1'
Seting catalog search parameters based on the expected field of view 939.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013043 (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 0.010434 (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 960 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: 0.59"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.60"
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 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.60"
Estimated accuracy of the plate solution: 0.67"
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_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits -region wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits'
Saving fully-calibrated image wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits'
Saving fully-calibrated image wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits'
Saving fully-calibrated image wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits'
Preparing the HTML report for the field Cyg-07-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out34152.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out34329.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out34514.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out34532.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out34983.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out10857.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: 2s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32186_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
The candidate 32186_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381 did not pass the final checks
**** FOUND 21:51:19.36 +36:49:38.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32666_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
The candidate 32666_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381 did not pass the final checks
**** FOUND 21:48:31.45 +42:05:27.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34152_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
The candidate 34152_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381 did not pass the final checks
**** FOUND 21:39:52.75 +41:57:44.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.82, MAG_FAINT_SEARCH_LIMIT=12.80)GAIADR2_OUTPUT=# 0.539 1966808809250286976 324.96999208243 +41.96243116639 11.6624 11.2064 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.539#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34329_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
The candidate 34329_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381 did not pass the final checks
**** FOUND 21:50:15.70 +35:39:34.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.98, MAG_FAINT_SEARCH_LIMIT=12.96)GAIADR2_OUTPUT=# 0.753 1949260878546849536 327.56564057233 +35.65960337615 11.4772 10.4690 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.753#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34514_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
The candidate 34514_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381 did not pass the final checks
**** FOUND 22:00:05.36 +40:01:43.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 0.716 1959247433424292096 330.02208478864 +40.02889147301 11.7811 10.8638 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.716#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34532_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
The candidate 34532_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381 did not pass the final checks
**** FOUND 21:24:56.07 +37:11:15.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.98, MAG_FAINT_SEARCH_LIMIT=12.96)GAIADR2_OUTPUT=# 5.256 1963793261174257152 321.23536600714 +37.18820597676 12.2607 11.8353 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.256#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34641_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
The candidate 34641_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381 did not pass the final checks
**** FOUND 21:42:59.52 +37:36:08.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34983_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
The candidate 34983_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381 did not pass the final checks
**** FOUND 21:42:51.46 +41:31:30.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.24, MAG_FAINT_SEARCH_LIMIT=13.22)GAIADR2_OUTPUT=# 2.894 1966541967219235712 325.71543458470 +41.52531179877 12.3657 11.7782 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.894#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10857_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 10857_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 6s
Prepared the HTML report for the field Cyg-07-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 ####
22:12:51.19 +39:09:59.7
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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits
SExtractor catalog cache: saved Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits.cat to cache
SExtractor catalog cache: saved Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits
Creating symlink local_wcs_cache/wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
Creating symlink local_wcs_cache/wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits
Creating symlink local_wcs_cache/wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits exists and is non-empty
wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits exists and is non-empty
wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits exists and is non-empty
wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits exists and is non-empty
The image scale is 5.78"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.7"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 21:48:48.775 +38:01:54.18
Second-epoch image center 21:49:09.074 +37:57:50.35
Angular distance between the image centers 0.10 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 21:48:48.775 +38:01:54.18
Second-epoch image center 21:49:08.467 +37:58:16.06
Angular distance between the image centers 0.09 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 21:49:09.074 +37:57:50.35
Second-epoch second image center 21:49:08.467 +37:58:16.06
Angular distance between the image centers 0.00741 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits &> /tmp/tmp.GhStFO5wJM
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits &> /tmp/tmp.FaFRqCqpb7
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits &> /tmp/tmp.oAiI7pQOac
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits &> /tmp/tmp.QJKpEURt43
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits and wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits and wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits.cat
Found non-empty wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits and wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits.cat
The reference image (wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits) and catalog (wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits.cat) found
'wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.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-2 149 out of 201016 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 20.958293
a=0.000000 b=1.000000 c=20.958293
From vast_summary.log: estimated ref. image limiting mag.: -7.43
Updating vast_summary.log: Estimated ref. image limiting mag.: 13.53
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 13.53
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 97 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits
2.1 pix Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
2.5 pix fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits
2.5 pix fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits
Limiting magnitude estimates:
13.5 mag. Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits
13.5 mag. Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
12.9 mag. fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits
12.9 mag. fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits
All-image limiting magnitude estimate: 12.9 (SNR ) 12.3 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.GhStFO5wJM (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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.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_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits' -> 'wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits
WCS_IMAGE_NAME=wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits
WCS-calibrated image found: wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits
Checking if the catalog wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits.cat corresponding to the image wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits alredy exist and is non-empty...
Catalog wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits.cat corresponding to the image wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits
WCS catalog name: wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=45, blended=28576, passed=200971
Got 200971 stars (including 172048 good ones) from the SExtractor catalog wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits.cat
util/solve_plate_with_UCAC5 got 200971 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 923.2'
Seting catalog search parameters based on the expected field of view 923.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012822 (46.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010258 (36.9 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 369 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 4.37"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 5.09"
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 467 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 5.09"
Estimated accuracy of the plate solution: 5.74"
Excluding outliers - 413 stars left (next iteration limit 325)
The image catalog is written to wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits -region wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.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.FaFRqCqpb7 (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-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.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_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits 572.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.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-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.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-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits' -> 'wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
WCS_IMAGE_NAME=wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
WCS-calibrated image found: wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
Checking if the catalog wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat corresponding to the image wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits alredy exist and is non-empty...
Catalog wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat corresponding to the image wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
WCS catalog name: wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=65, blended=28738, passed=202040
Got 202040 stars (including 172959 good ones) from the SExtractor catalog wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat
util/solve_plate_with_UCAC5 got 202040 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 932.3'
Seting catalog search parameters based on the expected field of view 932.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012949 (46.6 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010359 (37.3 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 409 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 3.16"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 3.60"
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 485 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 3.59"
Estimated accuracy of the plate solution: 2.74"
Excluding outliers - 456 stars left (next iteration limit 405)
The image catalog is written to wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits -region wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.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.oAiI7pQOac (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_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.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_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits
WCS-calibrated image found: wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits
Checking if the catalog wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits
WCS catalog name: wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits.cat
SExtractor catalog parsing summary: zero_flux=1, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=17, blended=14835, passed=127397
Got 127397 stars (including 112405 good ones) from the SExtractor catalog wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits.cat
util/solve_plate_with_UCAC5 got 127397 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.1'
Seting catalog search parameters based on the expected field of view 939.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013043 (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 0.010434 (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 963 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: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.54"
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 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.54"
Estimated accuracy of the plate solution: 0.58"
Excluding outliers - 961 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits -region wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.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.QJKpEURt43 (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_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.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_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits
WCS-calibrated image found: wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits
Checking if the catalog wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits
WCS catalog name: wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=14905, passed=128552
Got 128552 stars (including 113504 good ones) from the SExtractor catalog wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits.cat
util/solve_plate_with_UCAC5 got 128552 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.1'
Seting catalog search parameters based on the expected field of view 939.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013043 (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 0.010434 (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 963 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: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.54"
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 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.54"
Estimated accuracy of the plate solution: 0.60"
Excluding outliers - 961 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits -region wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.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_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits
Saving fully-calibrated image wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.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_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
Saving fully-calibrated image wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.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_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-43-43_20.00sec_-14.90C_LIGHT_0380.fits
Saving fully-calibrated image wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.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_2026-03-22_CI_Cyg-07-Q2b1x1_065320_TTUQ2b1x1_22078_9W926RFK/wcs_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381.fits
Preparing the HTML report for the field Cyg-07-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out248086.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out138402.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out219051.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226817.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226837.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226847.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226853.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226855.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226869.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226877.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226880.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226895.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226897.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226900.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226902.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226907.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226912.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226914.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226915.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226918.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226919.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226922.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226925.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226927.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226929.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226931.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out230956.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out231548.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out232119.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out232441.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234231.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234605.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234624.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235605.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235690.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236014.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236853.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236861.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237036.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237125.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237159.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237276.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237828.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out238660.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out239102.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out239556.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out239568.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out239591.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out239616.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out240010.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out240101.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out240248.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out240432.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out240483.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out240644.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out240726.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out241251.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out241296.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out241822.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out241934.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out241958.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out242081.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out242217.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out242279.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out242852.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out242886.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out243061.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out243282.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out243731.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out243734.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out244171.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out244614.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out244680.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out244827.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out245225.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out245628.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out245986.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246527.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247044.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248119.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248220.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248338.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248477.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248507.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out72103.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 140s
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: 47s
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Considering the candidate 226817_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 226817_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 226837_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 226837_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 226847_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 226847_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 226853_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 226853_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 226855_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 226855_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 226869_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 226869_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 226877_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 226877_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 226880_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 226880_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 226895_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 226895_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 226897_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 226897_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 226900_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 226900_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 226902_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 226902_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 226907_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 226907_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 226912_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 226912_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 226914_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 226914_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 226915_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 226915_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 226916_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
The candidate 226916_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381 did not pass the final checks
Rejecting candidate due to large distance (16.0") between the two second-epoch detections
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Considering the candidate 226918_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 226918_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 226919_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 226919_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 226922_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 226922_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 226925_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 226925_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 226927_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 226927_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 226929_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 226929_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 226931_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 226931_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 230956_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 230956_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 231548_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 231548_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 232119_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 232119_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 232441_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 232441_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 234231_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 234231_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 234605_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 234605_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 234624_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 234624_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 235605_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 235605_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 235690_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 235690_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 236014_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 236014_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 236209_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
The candidate 236209_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381 did not pass the final checks
**** FOUND 21:48:22.58 +38:40:00.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 236853_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 236853_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 236861_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 236861_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 237036_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 237036_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 237125_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 237125_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 237159_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 237159_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 237276_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 237276_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 237828_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 237828_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 237996_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
The candidate 237996_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381 did not pass the final checks
**** FOUND 21:51:46.06 +41:39:32.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 238660_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 238660_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 239102_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 239102_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 239510_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
The candidate 239510_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381 did not pass the final checks
**** FOUND 22:09:21.09 +33:46:49.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 239556_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 239556_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 239568_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 239568_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 239591_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 239591_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 239616_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 239616_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 240010_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 240010_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 240101_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 240101_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 240248_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 240248_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 240432_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 240432_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 240483_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 240483_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 240644_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 240644_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 240726_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 240726_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 241251_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 241251_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 241296_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 241296_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 241822_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 241822_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 241934_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 241934_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 241958_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 241958_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 242081_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 242081_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 242217_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 242217_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 242279_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 242279_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 242852_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 242852_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 242886_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 242886_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 243061_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 243061_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 243282_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 243282_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 243690_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
The candidate 243690_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381 did not pass the final checks
**** FOUND 21:47:58.45 +36:34:49.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 243731_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 243731_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 243734_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 243734_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 244171_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 244171_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 244614_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 244614_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 244680_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 244680_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 244827_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 244827_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 245225_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 245225_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 245628_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 245628_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 245986_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 245986_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 246527_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 246527_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 247044_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 247044_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 248086_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
The candidate 248086_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381 did not pass the final checks
**** FOUND 21:21:27.76 +37:08:10.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.52, MAG_FAINT_SEARCH_LIMIT=13.50)GAIADR2_OUTPUT=# 0.697 1963899707643448448 320.36580516621 +37.13649250162 13.4013 12.0717 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.697#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248119_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 248119_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 248220_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 248220_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 248338_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 248338_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 248477_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 248477_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 248507_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 248507_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 248566_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
The candidate 248566_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381 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 219051_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 219051_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
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Considering the candidate 76443_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
The candidate 76443_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381 did not pass the final checks
**** FOUND 22:12:51.16 +39:09:59.7 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 129504_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
The candidate 129504_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381 did not pass the final checks
**** FOUND 21:51:19.37 +36:49:38.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 47611_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
The candidate 47611_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381 did not pass the final checks
**** FOUND 21:49:56.74 +40:56:30.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 27577_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
The candidate 27577_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381 did not pass the final checks
Rejecting candidate due to large distance (26.7") between the two second-epoch detections
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Considering the candidate 138402_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 138402_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24612_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
The candidate 24612_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381 did not pass the final checks
**** FOUND 21:48:31.47 +42:05:28.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 145877_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
The candidate 145877_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381 did not pass the final checks
Rejecting candidate due to large distance (27.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72103_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
Preparing report for the candidate 72103_fd_Cyg-07-Q2b1x1_2026-03-22_05-44-31_20.00sec_-14.90C_LIGHT_0381
make_report_in_HTML.sh Phase 2 (HTML assembly): 16s
make_report_in_HTML.sh TOTAL: 203s
Prepared the HTML report for the field Cyg-07-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
22:12:51.19 +39:09:59.7
21:56:38.07 +36:20:35.0
22:03:42.55 +35:43:47.3
21:32:45.89 +37:06:35.6
21:54:20.75 +40:56:10.6
21:19:27.97 +36:07:29.4
21:25:28.13 +34:19:08.3
21:44:37.49 +38:02:16.8
21:20:00.27 +38:24:38.4
21:31:04.47 +40:43:44.2
21:36:13.70 +40:51:40.8
21:19:40.96 +35:26:24.6
21:27:41.77 +38:45:47.0
22:16:20.03 +38:24:01.4
21:48:12.45 +41:41:13.0
21:18:47.25 +38:10:23.0
21:23:43.93 +35:58:31.6
21:28:46.84 +42:05:19.7
21:27:24.06 +33:39:58.6
21:19:57.91 +39:52:34.6
21:41:05.58 +41:56:41.8
21:22:57.05 +34:21:07.1
21:18:16.67 +37:55:33.8
21:46:27.06 +42:00:04.1
22:14:06.05 +39:37:06.3
21:27:38.48 +37:49:02.3
21:47:57.29 +36:35:34.4
21:42:55.13 +41:10:18.7
21:31:14.77 +39:26:59.5
21:42:50.23 +37:29:34.1
21:52:09.50 +38:58:10.4
21:35:04.73 +40:51:23.3
22:13:14.49 +41:47:44.0
22:08:10.05 +37:08:03.6
21:33:36.31 +38:32:49.9
22:07:50.33 +40:07:28.7
21:31:28.50 +35:34:31.7
21:55:05.22 +34:46:32.0
21:42:56.20 +37:35:03.8
22:11:22.97 +39:44:16.4
21:18:39.97 +39:14:37.5
21:42:50.12 +38:10:46.0
21:35:30.55 +34:46:53.3
22:00:54.54 +41:16:15.5
22:02:40.16 +38:06:49.0
22:14:09.52 +38:28:30.5
21:23:19.17 +35:13:34.5
21:44:49.77 +36:56:56.3
21:49:54.63 +34:54:45.1
21:41:14.03 +41:15:46.6
21:59:27.32 +38:47:14.0
22:21:21.24 +41:17:36.1
22:03:59.96 +39:46:43.0
22:13:05.33 +41:48:42.2
21:57:20.66 +40:56:59.8
22:13:03.51 +38:28:18.7
22:13:03.62 +38:27:57.2
22:02:27.76 +42:04:06.0
21:58:15.43 +41:40:34.9
22:06:31.82 +34:33:33.6
21:59:28.72 +37:59:48.7
22:15:17.48 +39:47:55.2
21:50:11.33 +35:33:10.6
22:00:00.02 +38:42:25.7
21:42:24.37 +38:38:05.5
22:07:43.23 +37:37:05.9
22:04:36.75 +38:54:17.0
22:03:22.55 +37:41:21.5
21:41:09.79 +36:39:10.0
21:52:31.15 +41:28:59.4
22:06:04.04 +39:59:13.9
21:50:34.13 +37:11:05.5
21:56:00.49 +37:10:59.3
21:46:36.53 +37:39:36.9
21:31:28.73 +34:33:30.5
21:37:55.36 +36:14:23.5
21:41:50.91 +35:55:33.8
21:51:42.39 +41:44:43.6
21:43:03.21 +37:32:32.8
21:50:24.65 +34:50:30.3
21:50:58.68 +36:44:37.8
21:28:20.89 +36:09:01.6
21:24:37.60 +35:22:22.9
21:58:42.44 +41:08:27.9
21:50:52.42 +39:37:43.0
########### Completed Cyg-07-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 ####
22:12:51.19 +39:09:59.7
21:32:45.89 +37:06:35.6
21:54:20.75 +40:56:10.6
21:19:27.97 +36:07:29.4
21:25:28.13 +34:19:08.3
21:44:37.49 +38:02:16.8
21:20:00.27 +38:24:38.4
21:31:04.47 +40:43:44.2
21:36:13.70 +40:51:40.8
21:19:40.96 +35:26:24.6
21:27:41.77 +38:45:47.0
22:16:20.03 +38:24:01.4
21:48:12.45 +41:41:13.0
21:18:47.25 +38:10:23.0
21:23:43.93 +35:58:31.6
21:28:46.84 +42:05:19.7
21:27:24.06 +33:39:58.6
21:19:57.91 +39:52:34.6
21:41:05.58 +41:56:41.8
21:22:57.05 +34:21:07.1
21:18:16.67 +37:55:33.8
21:46:27.06 +42:00:04.1
22:14:06.05 +39:37:06.3
21:27:38.48 +37:49:02.3
21:47:57.29 +36:35:34.4
21:42:55.13 +41:10:18.7
21:31:14.77 +39:26:59.5
21:42:50.23 +37:29:34.1
21:52:09.50 +38:58:10.4
21:35:04.73 +40:51:23.3
22:13:14.49 +41:47:44.0
22:08:10.05 +37:08:03.6
21:33:36.31 +38:32:49.9
22:07:50.33 +40:07:28.7
21:31:28.50 +35:34:31.7
21:55:05.22 +34:46:32.0
21:42:56.20 +37:35:03.8
22:11:22.97 +39:44:16.4
21:18:39.97 +39:14:37.5
21:42:50.12 +38:10:46.0
21:35:30.55 +34:46:53.3
22:00:54.54 +41:16:15.5
22:02:40.16 +38:06:49.0
22:14:09.52 +38:28:30.5
21:23:19.17 +35:13:34.5
21:44:49.77 +36:56:56.3
21:49:54.63 +34:54:45.1
21:41:14.03 +41:15:46.6
21:59:27.32 +38:47:14.0
22:21:21.24 +41:17:36.1
22:03:59.96 +39:46:43.0
22:13:05.33 +41:48:42.2
21:57:20.66 +40:56:59.8
22:13:03.51 +38:28:18.7
22:13:03.62 +38:27:57.2
22:02:27.76 +42:04:06.0
21:58:15.43 +41:40:34.9
22:06:31.82 +34:33:33.6
21:59:28.72 +37:59:48.7
22:15:17.48 +39:47:55.2
21:50:11.33 +35:33:10.6
22:00:00.02 +38:42:25.7
21:42:24.37 +38:38:05.5
22:07:43.23 +37:37:05.9
22:04:36.75 +38:54:17.0
22:03:22.55 +37:41:21.5
21:41:09.79 +36:39:10.0
21:52:31.15 +41:28:59.4
22:06:04.04 +39:59:13.9
21:50:34.13 +37:11:05.5
21:56:00.49 +37:10:59.3
21:46:36.53 +37:39:36.9
21:31:28.73 +34:33:30.5
21:37:55.36 +36:14:23.5
21:41:50.91 +35:55:33.8
21:51:42.39 +41:44:43.6
21:43:03.21 +37:32:32.8
21:50:24.65 +34:50:30.3
21:50:58.68 +36:44:37.8
21:28:20.89 +36:09:01.6
21:24:37.60 +35:22:22.9
21:58:42.44 +41:08:27.9
22:03:42.55 +35:43:47.3
21:56:38.07 +36:20:35.0
21:50:52.42 +39:37:43.0
###################################################################################
22:12:51.19 +39:09:59.7 -- not an asteroid (will add it to exclusion list)
21:32:45.89 +37:06:35.6 -- not an asteroid (will add it to exclusion list)
21:54:20.75 +40:56:10.6 -- not an asteroid (will add it to exclusion list)
21:19:27.97 +36:07:29.4 -- not an asteroid (will add it to exclusion list)
21:25:28.13 +34:19:08.3 -- not an asteroid (will add it to exclusion list)
21:44:37.49 +38:02:16.8 -- not an asteroid (will add it to exclusion list)
21:20:00.27 +38:24:38.4 -- not an asteroid (will add it to exclusion list)
21:31:04.47 +40:43:44.2 -- not an asteroid (will add it to exclusion list)
21:36:13.70 +40:51:40.8 -- not an asteroid (will add it to exclusion list)
21:19:40.96 +35:26:24.6 -- not an asteroid (will add it to exclusion list)
21:27:41.77 +38:45:47.0 -- not an asteroid (will add it to exclusion list)
22:16:20.03 +38:24:01.4 -- not an asteroid (will add it to exclusion list)
21:48:12.45 +41:41:13.0 -- not an asteroid (will add it to exclusion list)
21:18:47.25 +38:10:23.0 -- not an asteroid (will add it to exclusion list)
21:23:43.93 +35:58:31.6 -- not an asteroid (will add it to exclusion list)
21:28:46.84 +42:05:19.7 -- not an asteroid (will add it to exclusion list)
21:27:24.06 +33:39:58.6 -- not an asteroid (will add it to exclusion list)
21:19:57.91 +39:52:34.6 -- not an asteroid (will add it to exclusion list)
21:41:05.58 +41:56:41.8 -- not an asteroid (will add it to exclusion list)
21:22:57.05 +34:21:07.1 -- not an asteroid (will add it to exclusion list)
21:18:16.67 +37:55:33.8 -- not an asteroid (will add it to exclusion list)
21:46:27.06 +42:00:04.1 -- not an asteroid (will add it to exclusion list)
22:14:06.05 +39:37:06.3 -- not an asteroid (will add it to exclusion list)
21:27:38.48 +37:49:02.3 -- not an asteroid (will add it to exclusion list)
21:47:57.29 +36:35:34.4 -- not an asteroid (will add it to exclusion list)
21:42:55.13 +41:10:18.7 -- not an asteroid (will add it to exclusion list)
21:31:14.77 +39:26:59.5 -- not an asteroid (will add it to exclusion list)
21:42:50.23 +37:29:34.1 -- not an asteroid (will add it to exclusion list)
21:52:09.50 +38:58:10.4 -- not an asteroid (will add it to exclusion list)
21:35:04.73 +40:51:23.3 -- not an asteroid (will add it to exclusion list)
22:13:14.49 +41:47:44.0 -- not an asteroid (will add it to exclusion list)
22:08:10.05 +37:08:03.6 -- not an asteroid (will add it to exclusion list)
21:33:36.31 +38:32:49.9 -- not an asteroid (will add it to exclusion list)
22:07:50.33 +40:07:28.7 -- not an asteroid (will add it to exclusion list)
21:31:28.50 +35:34:31.7 -- not an asteroid (will add it to exclusion list)
21:55:05.22 +34:46:32.0 -- not an asteroid (will add it to exclusion list)
21:42:56.20 +37:35:03.8 -- not an asteroid (will add it to exclusion list)
22:11:22.97 +39:44:16.4 -- not an asteroid (will add it to exclusion list)
21:18:39.97 +39:14:37.5 -- not an asteroid (will add it to exclusion list)
21:42:50.12 +38:10:46.0 -- not an asteroid (will add it to exclusion list)
21:35:30.55 +34:46:53.3 -- not an asteroid (will add it to exclusion list)
22:00:54.54 +41:16:15.5 -- not an asteroid (will add it to exclusion list)
22:02:40.16 +38:06:49.0 -- not an asteroid (will add it to exclusion list)
22:14:09.52 +38:28:30.5 -- not an asteroid (will add it to exclusion list)
21:23:19.17 +35:13:34.5 -- not an asteroid (will add it to exclusion list)
21:44:49.77 +36:56:56.3 -- not an asteroid (will add it to exclusion list)
21:49:54.63 +34:54:45.1 -- not an asteroid (will add it to exclusion list)
21:41:14.03 +41:15:46.6 -- not an asteroid (will add it to exclusion list)
21:59:27.32 +38:47:14.0 -- not an asteroid (will add it to exclusion list)
22:21:21.24 +41:17:36.1 -- not an asteroid (will add it to exclusion list)
22:03:59.96 +39:46:43.0 -- not an asteroid (will add it to exclusion list)
22:13:05.33 +41:48:42.2 -- not an asteroid (will add it to exclusion list)
21:57:20.66 +40:56:59.8 -- not an asteroid (will add it to exclusion list)
22:13:03.51 +38:28:18.7 -- not an asteroid (will add it to exclusion list)
22:13:03.62 +38:27:57.2 -- not an asteroid (will add it to exclusion list)
22:02:27.76 +42:04:06.0 -- not an asteroid (will add it to exclusion list)
21:58:15.43 +41:40:34.9 -- not an asteroid (will add it to exclusion list)
22:06:31.82 +34:33:33.6 -- not an asteroid (will add it to exclusion list)
21:59:28.72 +37:59:48.7 -- not an asteroid (will add it to exclusion list)
22:15:17.48 +39:47:55.2 -- not an asteroid (will add it to exclusion list)
21:50:11.33 +35:33:10.6 -- not an asteroid (will add it to exclusion list)
22:00:00.02 +38:42:25.7 -- not an asteroid (will add it to exclusion list)
21:42:24.37 +38:38:05.5 -- not an asteroid (will add it to exclusion list)
22:07:43.23 +37:37:05.9 -- not an asteroid (will add it to exclusion list)
22:04:36.75 +38:54:17.0 -- not an asteroid (will add it to exclusion list)
22:03:22.55 +37:41:21.5 -- not an asteroid (will add it to exclusion list)
21:41:09.79 +36:39:10.0 -- not an asteroid (will add it to exclusion list)
21:52:31.15 +41:28:59.4 -- not an asteroid (will add it to exclusion list)
22:06:04.04 +39:59:13.9 -- not an asteroid (will add it to exclusion list)
21:50:34.13 +37:11:05.5 -- not an asteroid (will add it to exclusion list)
21:56:00.49 +37:10:59.3 -- not an asteroid (will add it to exclusion list)
21:46:36.53 +37:39:36.9 -- not an asteroid (will add it to exclusion list)
21:31:28.73 +34:33:30.5 -- not an asteroid (will add it to exclusion list)
21:37:55.36 +36:14:23.5 -- not an asteroid (will add it to exclusion list)
21:41:50.91 +35:55:33.8 -- not an asteroid (will add it to exclusion list)
21:51:42.39 +41:44:43.6 -- not an asteroid (will add it to exclusion list)
21:43:03.21 +37:32:32.8 -- not an asteroid (will add it to exclusion list)
21:50:24.65 +34:50:30.3 -- not an asteroid (will add it to exclusion list)
21:50:58.68 +36:44:37.8 -- not an asteroid (will add it to exclusion list)
21:28:20.89 +36:09:01.6 -- not an asteroid (will add it to exclusion list)
21:24:37.60 +35:22:22.9 -- not an asteroid (will add it to exclusion list)
21:58:42.44 +41:08:27.9 -- not an asteroid (will add it to exclusion list)
22:03:42.55 +35:43:47.3 -- not an asteroid (will add it to exclusion list)
21:56:38.07 +36:20:35.0 -- not an asteroid (will add it to exclusion list)
21:50:52.42 +39:37:43.0 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
21:18:16.67 +37:55:33.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:18:39.97 +39:14:37.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:18:47.25 +38:10:23.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:19:27.97 +36:07:29.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:19:40.96 +35:26:24.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:19:57.91 +39:52:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:20:00.27 +38:24:38.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:22:57.05 +34:21:07.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:23:19.17 +35:13:34.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:23:43.93 +35:58:31.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:24:37.60 +35:22:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:25:28.13 +34:19:08.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:24.06 +33:39:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:38.48 +37:49:02.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:41.77 +38:45:47.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:20.89 +36:09:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:46.84 +42:05:19.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:04.47 +40:43:44.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:14.77 +39:26:59.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:28.50 +35:34:31.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:28.73 +34:33:30.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:45.89 +37:06:35.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:33:36.31 +38:32:49.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:04.73 +40:51:23.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:30.55 +34:46:53.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:13.70 +40:51:40.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:55.36 +36:14:23.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:05.58 +41:56:41.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:09.79 +36:39:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:14.03 +41:15:46.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:50.91 +35:55:33.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:24.37 +38:38:05.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:50.12 +38:10:46.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:50.23 +37:29:34.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:55.13 +41:10:18.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:56.20 +37:35:03.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:03.21 +37:32:32.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:37.49 +38:02:16.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:49.77 +36:56:56.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:27.06 +42:00:04.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:36.53 +37:39:36.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:47:57.29 +36:35:34.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:48:12.45 +41:41:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:54.63 +34:54:45.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:11.33 +35:33:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:24.65 +34:50:30.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:34.13 +37:11:05.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:52.42 +39:37:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:58.68 +36:44:37.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:51:42.39 +41:44:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:52:09.50 +38:58:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:52:31.15 +41:28:59.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:54:20.75 +40:56:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:55:05.22 +34:46:32.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:00.49 +37:10:59.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:38.07 +36:20:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:57:20.66 +40:56:59.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:15.43 +41:40:34.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:42.44 +41:08:27.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:27.32 +38:47:14.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:28.72 +37:59:48.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:00:00.02 +38:42:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:00:54.54 +41:16:15.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:27.76 +42:04:06.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:40.16 +38:06:49.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:03:22.55 +37:41:21.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:03:42.55 +35:43:47.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:03:59.96 +39:46:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:04:36.75 +38:54:17.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:06:04.04 +39:59:13.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:06:31.82 +34:33:33.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:07:43.23 +37:37:05.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:07:50.33 +40:07:28.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:08:10.05 +37:08:03.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:11:22.97 +39:44:16.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:12:51.19 +39:09:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:13:03.51 +38:28:18.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:13:03.62 +38:27:57.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:13:05.33 +41:48:42.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:13:14.49 +41:47:44.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:14:06.05 +39:37:06.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:14:09.52 +38:28:30.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:15:17.48 +39:47:55.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:16:20.03 +38:24:01.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:21:21.24 +41:17:36.1 -- 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)
21:18:16.67 +37:55:33.8 -- a known variable star
21:18:39.97 +39:14:37.5 -- not a known variable star
21:18:47.25 +38:10:23.0 -- a known variable star
21:19:27.97 +36:07:29.4 -- not a known variable star
21:19:40.96 +35:26:24.6 -- not a known variable star
21:19:57.91 +39:52:34.6 -- not a known variable star
21:20:00.27 +38:24:38.4 -- a known variable star
21:22:57.05 +34:21:07.1 -- not a known variable star
21:23:19.17 +35:13:34.5 -- not a known variable star
21:23:43.93 +35:58:31.6 -- not a known variable star
21:24:37.60 +35:22:22.9 -- a known variable star
21:25:28.13 +34:19:08.3 -- not a known variable star
21:27:24.06 +33:39:58.6 -- not a known variable star
21:27:38.48 +37:49:02.3 -- not a known variable star
21:27:41.77 +38:45:47.0 -- not a known variable star
21:28:20.89 +36:09:01.6 -- not a known variable star
21:28:46.84 +42:05:19.7 -- not a known variable star
21:31:04.47 +40:43:44.2 -- not a known variable star
21:31:14.77 +39:26:59.5 -- a known variable star
21:31:28.50 +35:34:31.7 -- not a known variable star
21:31:28.73 +34:33:30.5 -- not a known variable star
21:32:45.89 +37:06:35.6 -- not a known variable star
21:33:36.31 +38:32:49.9 -- not a known variable star
21:35:04.73 +40:51:23.3 -- a known variable star
21:35:30.55 +34:46:53.3 -- not a known variable star
21:36:13.70 +40:51:40.8 -- not a known variable star
21:37:55.36 +36:14:23.5 -- not a known variable star
21:41:05.58 +41:56:41.8 -- a known variable star
21:41:09.79 +36:39:10.0 -- a known variable star
21:41:14.03 +41:15:46.6 -- not a known variable star
21:41:50.91 +35:55:33.8 -- not a known variable star
21:42:24.37 +38:38:05.5 -- not a known variable star
21:42:50.12 +38:10:46.0 -- not a known variable star
21:42:50.23 +37:29:34.1 -- a known variable star
21:42:55.13 +41:10:18.7 -- not a known variable star
21:42:56.20 +37:35:03.8 -- a known variable star
21:43:03.21 +37:32:32.8 -- not a known variable star
21:44:37.49 +38:02:16.8 -- not a known variable star
21:44:49.77 +36:56:56.3 -- not a known variable star
21:46:27.06 +42:00:04.1 -- not a known variable star
21:46:36.53 +37:39:36.9 -- not a known variable star
21:47:57.29 +36:35:34.4 -- not a known variable star
21:48:12.45 +41:41:13.0 -- not a known variable star
21:49:54.63 +34:54:45.1 -- not a known variable star
21:50:11.33 +35:33:10.6 -- a known variable star
21:50:24.65 +34:50:30.3 -- not a known variable star
21:50:34.13 +37:11:05.5 -- not a known variable star
21:50:52.42 +39:37:43.0 -- not a known variable star
21:50:58.68 +36:44:37.8 -- not a known variable star
21:51:42.39 +41:44:43.6 -- a known variable star
21:52:09.50 +38:58:10.4 -- not a known variable star
21:52:31.15 +41:28:59.4 -- not a known variable star
21:54:20.75 +40:56:10.6 -- not a known variable star
21:55:05.22 +34:46:32.0 -- not a known variable star
21:56:00.49 +37:10:59.3 -- not a known variable star
21:56:38.07 +36:20:35.0 -- a known variable star
21:57:20.66 +40:56:59.8 -- not a known variable star
21:58:15.43 +41:40:34.9 -- not a known variable star
21:58:42.44 +41:08:27.9 -- not a known variable star
21:59:27.32 +38:47:14.0 -- not a known variable star
21:59:28.72 +37:59:48.7 -- not a known variable star
22:00:00.02 +38:42:25.7 -- a known variable star
22:00:54.54 +41:16:15.5 -- not a known variable star
22:02:27.76 +42:04:06.0 -- not a known variable star
22:02:40.16 +38:06:49.0 -- not a known variable star
22:03:22.55 +37:41:21.5 -- not a known variable star
22:03:42.55 +35:43:47.3 -- a known variable star
22:03:59.96 +39:46:43.0 -- not a known variable star
22:04:36.75 +38:54:17.0 -- not a known variable star
22:06:04.04 +39:59:13.9 -- not a known variable star
22:06:31.82 +34:33:33.6 -- not a known variable star
22:07:43.23 +37:37:05.9 -- not a known variable star
22:07:50.33 +40:07:28.7 -- not a known variable star
22:08:10.05 +37:08:03.6 -- not a known variable star
22:11:22.97 +39:44:16.4 -- not a known variable star
22:12:51.19 +39:09:59.7 -- a known variable star
22:13:03.51 +38:28:18.7 -- not a known variable star
22:13:03.62 +38:27:57.2 -- not a known variable star
22:13:05.33 +41:48:42.2 -- not a known variable star
22:13:14.49 +41:47:44.0 -- not a known variable star
22:14:06.05 +39:37:06.3 -- not a known variable star
22:14:09.52 +38:28:30.5 -- a known variable star
22:15:17.48 +39:47:55.2 -- not a known variable star
22:16:20.03 +38:24:01.4 -- not a known variable star
22:21:21.24 +41:17:36.1 -- not a known variable star
Found 68 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
85 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 85 (excluding asteroids and hot pixels), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is 500
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461121.94714414 -observatory 500
22:38:41.50 -07:55:26.2 Mercury (0.9mag)
01:13:10.12 +06:52:28.4 Venus (-3.9mag)
23:07:23.30 -06:47:46.6 Mars (1.2mag)
07:04:58.56 +22:57:45.1 Jupiter (-2.3mag)
00:18:00.70 -00:21:53.8 Saturn (0.9mag)
03:43:09.43 +19:32:37.1 Uranus (5.8mag)
00:07:29.48 -00:36:44.4 Neptune (7.8mag)
20:32:08.00 -22:53:36.3 Pluto (14.5mag)
02:50:37.25 +21:26:57.3 Moon (-9.2mag)
-rw-r--r-- 1 apache apache 361 Mar 22 08:02 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461121.94714414:
07:05:02.50 +22:57:40.1 Io (5.6mag)
07:05:07.94 +22:57:29.1 Europa (5.7mag)
07:04:45.29 +22:58:16.3 Ganymede (5.2mag)
07:04:21.06 +22:58:55.4 Callisto (6.4mag)
07:08:59.47 +22:58:31.3 Himalia (15.2mag)
07:04:58.90 +22:57:47.0 Thebe (16.1mag)
07:08:36.13 +23:22:26.0 Elara (17.2mag)
07:02:12.22 +23:50:40.0 Pasiphae (17.2mag)
07:13:44.82 +22:52:28.2 Carme (18.3mag)
00:18:00.33 -00:21:57.5 Titan (8.8mag)
00:18:03.47 -00:21:41.8 Rhea (10.1mag)
00:18:29.05 -00:19:47.1 Iapetus (11.5mag)
00:18:15.74 -00:21:53.4 Hyperion (14.8mag)
00:19:54.06 -00:10:44.6 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Mar 22 08:03 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461121.94714414:
13:01:49.76 +07:18:19.5 JWST
18:42:01.20 +24:16:39.8 Chandra
18:52:45.42 -01:20:46.1 XMM-Newton
-rw-r--r-- 1 apache apache 96 Mar 22 08:02 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461121.94714414 -observatory 500
-rw-r--r-- 1 apache apache 0 Mar 22 08:02 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
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
11:44:44.19 -62:10:45.50 ASASSN-26bq 2026-03-15.03 15.31
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 -0.22
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
11:30:09.70 -47:26:45.00 ASASSN-26bn 2026-03-10.3 15.14
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
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
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
14:15:47.49 -48:05:16.60 SN2026dez 2026-02-19.31 15.91
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
13:01:07.22 -11:25:16.10 AT2026bzh 2026-02-12.16 17.22
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
05:14:22.36 -60:47:20.70 SN 2026apb 2026-01-24.08 17.35
06:39:26.57 -21:49:19.60 AT2026afe 2026-01-23.11 16.17
09:27:23.48 -32:00:31.10 SN 2023kuy 2026-01-21.24 15.33
09:38:44.42 -20:00:54.30 SN2026afi 2026-01-20.24 17.43
06:30:51.41 -74:35:46.80 AT2026ahr 2026-01-20.09 16.98
13:33:03.15 -16:14:28.70 SN2026amc 2026-01-20.29 16.9
06:57:11.13 -17:24:42.80 ASASSN-26an 2026-01-19.31 13.99
17:41:29.59 +68:57:34.90 2026abj 2026-01-18.64 17.02
10:22:25.13 +04:00:01.40 SN 2026kc 2026-01-18.24 16.4
12:42:03.30 +00:41:41.80 SN 2026pg 2026-01-18.5 17.44
-rw-r--r-- 1 apache apache 5.7K Mar 22 08:02 asassn_transients_list.txt
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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 22 08:02 tocp_transients_list.txt
