This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 03 27.3697 2461126.8697 12.49 19:40:01.06 +32:06:52.4
66.73505 4.80800 galactic Cyg Second-epoch detections are separated by 3.2" and 1.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J294.9955+32.1137 | 19:40:01.06 +32:06:52.4 (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 J294.9955+32.1137,2461126.8697,12.49,0.05,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
ATO J294.9955+32.1137 20260327.3697 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-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:40:01.06 +32:06:52.4 ;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-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20_00sec_-15_00C_LIGHT_0376_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20_00sec_-15_00C_LIGHT_0375_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20_00sec_-15_00C_LIGHT_0376_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20_00sec_-15_00C_LIGHT_0375_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J195543.93+321927.2,2461126.8697,12.42,0.05,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 J195543.93+321927.2 20260327.3697 12.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:55:44.73 +32:19:10.4 ;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-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20_00sec_-15_00C_LIGHT_0376_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20_00sec_-15_00C_LIGHT_0375_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20_00sec_-15_00C_LIGHT_0376_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20_00sec_-15_00C_LIGHT_0375_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.3697 2461126.8697 12.21 20:24:38.89 +29:13:54.1
69.38446 -4.85049 galactic Vul Second-epoch detections are separated by 2.2" and 0.8 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 1860487237442643072 | 20:24:38.88 +29:13:47.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1860487237442643072,2461126.8697,12.21,0.05,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
Gaia DR3 1860487237442643072 20260327.3697 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-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:24:38.89 +29:13:54.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20_00sec_-15_00C_LIGHT_0376_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20_00sec_-15_00C_LIGHT_0375_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20_00sec_-15_00C_LIGHT_0376_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20_00sec_-15_00C_LIGHT_0375_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
HAT 199-14347,2461126.8697,12.19,0.05,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
HAT 199-14347 20260327.3697 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:56:31.72 +33:53:49.6 ;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-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20_00sec_-15_00C_LIGHT_0376_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20_00sec_-15_00C_LIGHT_0375_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20_00sec_-15_00C_LIGHT_0376_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20_00sec_-15_00C_LIGHT_0375_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.3697 2461126.8697 12.31 19:29:34.95 +28:21:45.6
62.34619 4.98362 galactic Cyg Second-epoch detections are separated by 4.9" and 0.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2026187311935298816 | 19:29:33.74 +28:21:43.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2026187311935298816,2461126.8697,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2026187311935298816 20260327.3697 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:29:34.95 +28:21:45.6 ;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-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20_00sec_-15_00C_LIGHT_0376_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20_00sec_-15_00C_LIGHT_0375_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20_00sec_-15_00C_LIGHT_0376_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20_00sec_-15_00C_LIGHT_0375_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 1860316229026094336,2461126.8697,12.09,0.05,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
Gaia DR3 1860316229026094336 20260327.3697 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:25:47.57 +28:39:01.0 ;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-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20_00sec_-15_00C_LIGHT_0376_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20_00sec_-15_00C_LIGHT_0375_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20_00sec_-15_00C_LIGHT_0376_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20_00sec_-15_00C_LIGHT_0375_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J193223.71+311412.5,2461126.8697,12.26,0.05,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
ASASSN-V J193223.71+311412.5 20260327.3697 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-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:32:24.89 +31:14:26.8 ;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-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20_00sec_-15_00C_LIGHT_0376_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20_00sec_-15_00C_LIGHT_0375_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20_00sec_-15_00C_LIGHT_0376_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20_00sec_-15_00C_LIGHT_0375_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.3697 2461126.8697 12.15 19:33:33.79 +28:51:50.3
63.20593 4.45410 galactic Cyg Second-epoch detections are separated by 3.7" and 1.6 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 J293.3861+28.8632 | 19:33:32.68 +28:51:47.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J293.3861+28.8632,2461126.8697,12.15,0.05,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 J293.3861+28.8632 20260327.3697 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-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:33:33.79 +28:51:50.3 ;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-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20_00sec_-15_00C_LIGHT_0376_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20_00sec_-15_00C_LIGHT_0375_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20_00sec_-15_00C_LIGHT_0376_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20_00sec_-15_00C_LIGHT_0375_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
TY Cyg,2461126.8697,10.91,0.05,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
TY Cyg 20260327.3697 10.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:33:52.27 +28:19:44.3 ;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-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20_00sec_-15_00C_LIGHT_0376_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20_00sec_-15_00C_LIGHT_0375_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20_00sec_-15_00C_LIGHT_0376_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20_00sec_-15_00C_LIGHT_0375_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J193501.47+282217.7,2461126.8697,12.43,0.05,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
ZTF J193501.47+282217.7 20260327.3697 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-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:35:01.07 +28:22:16.8 ;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-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20_00sec_-15_00C_LIGHT_0376_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20_00sec_-15_00C_LIGHT_0375_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20_00sec_-15_00C_LIGHT_0376_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20_00sec_-15_00C_LIGHT_0375_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.3697 2461126.8697 12.21 19:49:13.77 +33:44:55.9
69.11919 3.93886 galactic Cyg Second-epoch detections are separated by 1.9" and 1.3 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 J297.3178+33.7435 | 19:49:13.92 +33:44:17.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J297.3178+33.7435,2461126.8697,12.21,0.05,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 J297.3178+33.7435 20260327.3697 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-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:49:13.77 +33:44:55.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20_00sec_-15_00C_LIGHT_0376_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20_00sec_-15_00C_LIGHT_0375_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20_00sec_-15_00C_LIGHT_0376_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20_00sec_-15_00C_LIGHT_0375_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.3697 2461126.8697 12.34 20:27:04.64 +30:17:21.1
70.55689 -4.67413 galactic Cyg Second-epoch detections are separated by 1.2" and 1.2 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 J306.7701+30.2967 | 20:27:04.80 +30:17:19.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J306.7701+30.2967,2461126.8697,12.34,0.05,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
ATO J306.7701+30.2967 20260327.3697 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-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:27:04.64 +30:17:21.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20_00sec_-15_00C_LIGHT_0376_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20_00sec_-15_00C_LIGHT_0375_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20_00sec_-15_00C_LIGHT_0376_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20_00sec_-15_00C_LIGHT_0375_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 2028814113928438656,2461126.8697,11.73,0.05,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
Gaia DR3 2028814113928438656 20260327.3697 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-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:52:10.20 +29:21:06.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20_00sec_-15_00C_LIGHT_0376_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20_00sec_-15_00C_LIGHT_0375_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20_00sec_-15_00C_LIGHT_0376_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20_00sec_-15_00C_LIGHT_0375_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J195012.13+274339.1,2461126.8697,12.09,0.05,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
ZTF J195012.13+274339.1 20260327.3697 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:50:12.84 +27:43:33.5 ;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-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20_00sec_-15_00C_LIGHT_0376_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20_00sec_-15_00C_LIGHT_0375_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20_00sec_-15_00C_LIGHT_0376_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20_00sec_-15_00C_LIGHT_0375_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.3697 2461126.8697 12.10 20:25:07.40 +32:06:59.2
71.81218 -3.27939 galactic Cyg Second-epoch detections are separated by 3.4" and 1.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J306.2823+32.1167 | 20:25:07.75 +32:06:59.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J306.2823+32.1167,2461126.8697,12.10,0.05,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 J306.2823+32.1167 20260327.3697 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:25:07.40 +32:06:59.2 ;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-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20_00sec_-15_00C_LIGHT_0376_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20_00sec_-15_00C_LIGHT_0375_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20_00sec_-15_00C_LIGHT_0376_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20_00sec_-15_00C_LIGHT_0375_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.3697 2461126.8697 12.35 20:25:48.67 +29:58:52.2
70.14604 -4.62788 galactic Cyg Second-epoch detections are separated by 1.9" and 0.9 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 J306.4463+29.9854 | 20:25:48.82 +29:58:52.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.746+/-0.026 (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 J306.4463+29.9854,2461126.8697,12.35,0.05,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
ATO J306.4463+29.9854 20260327.3697 12.35CV 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-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:25:48.67 +29:58:52.2 ;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-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20_00sec_-15_00C_LIGHT_0376_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20_00sec_-15_00C_LIGHT_0375_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20_00sec_-15_00C_LIGHT_0376_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20_00sec_-15_00C_LIGHT_0375_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.3697 2461126.8697 12.04 20:27:39.35 +33:04:48.1
72.90851 -3.15759 galactic Cyg Second-epoch detections are separated by 0.3" and 1.3 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 J306.9066+33.0694 | 20:27:39.44 +33:04:48.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.273+/-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 J306.9066+33.0694,2461126.8697,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J306.9066+33.0694 20260327.3697 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:27:39.35 +33:04:48.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20_00sec_-15_00C_LIGHT_0376_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20_00sec_-15_00C_LIGHT_0375_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20_00sec_-15_00C_LIGHT_0376_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20_00sec_-15_00C_LIGHT_0375_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.3697 2461126.8697 12.59 20:27:51.49 +31:48:04.7
71.89033 -3.93492 galactic Cyg Second-epoch detections are separated by 3.0" and 0.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J306.9557+31.8116 | 20:27:51.87 +31:48:11.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J306.9557+31.8116,2461126.8697,12.59,0.05,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 J306.9557+31.8116 20260327.3697 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:27:51.49 +31:48:04.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20_00sec_-15_00C_LIGHT_0376_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20_00sec_-15_00C_LIGHT_0375_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20_00sec_-15_00C_LIGHT_0376_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20_00sec_-15_00C_LIGHT_0375_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.3697 2461126.8697 12.19 20:27:49.84 +30:21:40.0
70.71010 -4.76515 galactic Cyg Second-epoch detections are separated by 1.6" and 1.1 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 1860960130519769984 | 20:27:49.76 +30:21:36.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1860960130519769984,2461126.8697,12.19,0.05,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
Gaia DR3 1860960130519769984 20260327.3697 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:27:49.84 +30:21:40.0 ;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-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20_00sec_-15_00C_LIGHT_0376_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20_00sec_-15_00C_LIGHT_0375_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20_00sec_-15_00C_LIGHT_0376_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20_00sec_-15_00C_LIGHT_0375_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: 2461098.99239403 27.02.2026 11:48:52.844 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
First image: 2461098.99239403 27.02.2026 11:48:52.844 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
Last image: 2461126.86999223 27.03.2026 08:52:37.329 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 25
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.95
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): 25024
Objects passed selection criteria: 24935
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 18467.8
Average stars matched: 17898 (96.9149 %)
Memory usage VmPeak: 130452 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Mar 27 04:00:12 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: 2461098.99239403 27.02.2026 11:48:52.844 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
First image: 2461098.99239403 27.02.2026 11:48:52.844 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
Last image: 2461126.86999223 27.03.2026 08:52:37.329 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 146
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.61
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: 43 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): 230335
Objects passed selection criteria: 229618
Measurements per detected object (mean, median, min, max): 2.5 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.5 2.0 2 4
Average stars detected per image: 158583
Average stars matched: 151975 (95.8334 %)
Memory usage VmPeak: 1992896 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Mar 27 04:06:43 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-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits
SExtractor catalog cache: saved Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat to cache
SExtractor catalog cache: saved Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.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-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461126.86950148
Plate-solving the images
'asassn_transients_list.txt' -> '../asassn_transients_list.txt'
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits exists and is non-empty
Saving wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits to local_wcs_cache/
'wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits' -> 'local_wcs_cache/wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits'
wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits exists and is non-empty
Saving wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits to local_wcs_cache/
'wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits' -> 'local_wcs_cache/wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits'
wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits exists and is non-empty
Saving wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits to local_wcs_cache/
'wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits' -> 'local_wcs_cache/wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits'
wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits exists and is non-empty
Saving wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits to local_wcs_cache/
'wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits' -> 'local_wcs_cache/wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 20:00:00.965 +30:00:24.17
Second-epoch image center 19:59:59.768 +29:58:52.88
Angular distance between the image centers 0.03 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 20:00:00.965 +30:00:24.17
Second-epoch image center 20:00:00.242 +29:58:50.23
Angular distance between the image centers 0.03 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 19:59:59.768 +29:58:52.88
Second-epoch second image center 20:00:00.242 +29:58:50.23
Angular distance between the image centers 0.00186 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-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits &> /tmp/tmp.DQmrbAe8yf
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits &> /tmp/tmp.NUzsBh4j9o
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits &> /tmp/tmp.tDrmBNVPON
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits &> /tmp/tmp.FSjPl1g7AM
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.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-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits and wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.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-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits and wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat
Found non-empty wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits and wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat
The reference image (wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits) and catalog (wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat) found
'wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.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 7455 out of 30878 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.854269
a=0.000000 b=1.000000 c=22.854269
From vast_summary.log: estimated ref. image limiting mag.: -7.95
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.90
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.90
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 15 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
2.0 pix Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
3.7 pix fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits
3.4 pix fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits
Limiting magnitude estimates:
14.9 mag. Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
14.9 mag. Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
13.5 mag. fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits
13.4 mag. fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits
All-image limiting magnitude estimate: 13.4 (SNR ) 10.9 (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.DQmrbAe8yf (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-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.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-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.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-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits' -> 'wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
WCS_IMAGE_NAME=wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
WCS-calibrated image found: wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
Checking if the catalog wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat corresponding to the image wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits alredy exist and is non-empty...
Catalog wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat corresponding to the image wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
WCS catalog name: wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3756, passed=30878
Got 30878 stars (including 27089 good ones) from the SExtractor catalog wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat
util/solve_plate_with_UCAC5 got 30878 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.1'
Seting catalog search parameters based on the expected field of view 942.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013085 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010468 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 700 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 1.90"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 2.54"
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 745 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 2.51"
Estimated accuracy of the plate solution: 2.18"
Excluding outliers - 698 stars left (next iteration limit 694)
The image catalog is written to wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits -region wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.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.NUzsBh4j9o (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-08-Q2b1x1_2026-02-27_05-49-53_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_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_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-08-Q2b1x1_2026-02-27_05-49-53_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-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_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-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits' -> 'wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
WCS_IMAGE_NAME=wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
WCS-calibrated image found: wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
Checking if the catalog wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat corresponding to the image wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits alredy exist and is non-empty...
Catalog wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat corresponding to the image wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_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-08-Q2b1x1_2026-02-27_05-49-53_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-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
WCS catalog name: wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_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=3771, passed=30931
Got 30931 stars (including 27121 good ones) from the SExtractor catalog wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat
util/solve_plate_with_UCAC5 got 30931 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010466 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 610 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 2.80"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 3.95"
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 654 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 3.91"
Estimated accuracy of the plate solution: 3.33"
Excluding outliers - 583 stars left (next iteration limit 586)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_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-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits -region wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_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.tDrmBNVPON (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits
WCS-calibrated image found: wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits
Checking if the catalog wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits.cat corresponding to the image wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits.cat corresponding to the image wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits
WCS catalog name: wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=447, passed=11183
Got 11183 stars (including 10734 good ones) from the SExtractor catalog wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits.cat
util/solve_plate_with_UCAC5 got 11183 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.2'
Seting catalog search parameters based on the expected field of view 939.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013044 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010436 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 932 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: 0.75"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.77"
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 932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.77"
Estimated accuracy of the plate solution: 0.81"
Excluding outliers - 921 stars left (next iteration limit 1013)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits -region wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.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.FSjPl1g7AM (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits
WCS-calibrated image found: wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits
Checking if the catalog wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits.cat corresponding to the image wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits.cat corresponding to the image wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits
WCS catalog name: wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=391, passed=10415
Got 10415 stars (including 10021 good ones) from the SExtractor catalog wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits.cat
util/solve_plate_with_UCAC5 got 10415 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 932 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: 0.68"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.73"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.73"
Estimated accuracy of the plate solution: 0.79"
Excluding outliers - 920 stars left (next iteration limit 1013)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits -region wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.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-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits'
Saving fully-calibrated image wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits'
Saving fully-calibrated image wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits'
Saving fully-calibrated image wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits'
Preparing the HTML report for the field Cyg-08-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06133_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 06133_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:51:30.92 +27:27:36.8 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12413_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 12413_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 20:03:38.80 +29:53:35.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16085_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 16085_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:58:38.14 +30:59:02.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19979_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 19979_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 20:04:36.11 +32:13:05.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06526_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 06526_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 20:01:06.23 +27:45:16.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08725_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 08725_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 20:14:14.40 +28:41:42.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04508_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 04508_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 20:10:33.50 +26:54:17.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04231_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 04231_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 20:11:47.93 +26:48:33.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06428_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 06428_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 20:15:45.86 +27:48:53.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24893_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 24893_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 20:15:23.69 +33:43:41.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14152_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 14152_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:39:22.89 +30:09:13.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 28999_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 28999_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:46:25.78 +33:43:27.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02583_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 02583_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:43:42.99 +25:46:20.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07969_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 07969_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:30:44.19 +27:57:41.7 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19717_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 19717_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 20:23:51.61 +32:11:23.9 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Cyg-08-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 ####
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-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits
SExtractor catalog cache: saved Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat to cache
SExtractor catalog cache: saved Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.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-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
Creating symlink local_wcs_cache/wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
Creating symlink local_wcs_cache/wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits
Creating symlink local_wcs_cache/wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.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-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits exists and is non-empty
wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits exists and is non-empty
wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits exists and is non-empty
wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 20:00:00.965 +30:00:24.17
Second-epoch image center 19:59:59.768 +29:58:52.88
Angular distance between the image centers 0.03 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 20:00:00.965 +30:00:24.17
Second-epoch image center 20:00:00.242 +29:58:50.23
Angular distance between the image centers 0.03 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 19:59:59.768 +29:58:52.88
Second-epoch second image center 20:00:00.242 +29:58:50.23
Angular distance between the image centers 0.00186 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-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits &> /tmp/tmp.jvL1dAag1Z
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits &> /tmp/tmp.36nVEZe0cb
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits &> /tmp/tmp.yhpB4oWQp8
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits &> /tmp/tmp.dHRBhfN6TY
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.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-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits and wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.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-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits and wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat
Found non-empty wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits and wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat
The reference image (wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits) and catalog (wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat) found
'wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.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 8842 out of 281578 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.629178
a=0.000000 b=1.000000 c=22.629178
From vast_summary.log: estimated ref. image limiting mag.: -7.61
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.02
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.02
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 101 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
1.9 pix Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
3.8 pix fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits
3.5 pix fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits
Limiting magnitude estimates:
15.0 mag. Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
15.0 mag. Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
13.5 mag. fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits
13.4 mag. fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits
All-image limiting magnitude estimate: 13.4 (SNR ) 12.7 (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.jvL1dAag1Z (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-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.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-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.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-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits' -> 'wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
WCS_IMAGE_NAME=wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
WCS-calibrated image found: wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
Checking if the catalog wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat corresponding to the image wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits alredy exist and is non-empty...
Catalog wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat corresponding to the image wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
WCS catalog name: wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=58, blended=51531, passed=281520
Got 281520 stars (including 229582 good ones) from the SExtractor catalog wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat
util/solve_plate_with_UCAC5 got 281520 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.1'
Seting catalog search parameters based on the expected field of view 942.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013085 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010468 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 692 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 2.01"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 2.27"
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 754 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 2.27"
Estimated accuracy of the plate solution: 1.36"
Excluding outliers - 713 stars left (next iteration limit 698)
The image catalog is written to wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits -region wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.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.36nVEZe0cb (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-08-Q2b1x1_2026-02-27_05-49-53_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_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_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-08-Q2b1x1_2026-02-27_05-49-53_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-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_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-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits' -> 'wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
WCS_IMAGE_NAME=wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
WCS-calibrated image found: wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
Checking if the catalog wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat corresponding to the image wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits alredy exist and is non-empty...
Catalog wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat corresponding to the image wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_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-08-Q2b1x1_2026-02-27_05-49-53_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-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
WCS catalog name: wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_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=61, blended=51082, passed=280646
Got 280646 stars (including 229187 good ones) from the SExtractor catalog wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat
util/solve_plate_with_UCAC5 got 280646 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010466 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 584 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 3.56"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 4.22"
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 627 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 4.22"
Estimated accuracy of the plate solution: 2.74"
Excluding outliers - 567 stars left (next iteration limit 568)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_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-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits -region wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_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.yhpB4oWQp8 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits
WCS-calibrated image found: wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits
Checking if the catalog wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits.cat corresponding to the image wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits.cat corresponding to the image wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits
WCS catalog name: wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=5939, passed=66113
Got 66113 stars (including 60124 good ones) from the SExtractor catalog wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits.cat
util/solve_plate_with_UCAC5 got 66113 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.2'
Seting catalog search parameters based on the expected field of view 939.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013044 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010436 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 931 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: 0.72"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.72"
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 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.72"
Estimated accuracy of the plate solution: 0.77"
Excluding outliers - 921 stars left (next iteration limit 1013)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits -region wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.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.dHRBhfN6TY (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits
WCS-calibrated image found: wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits
Checking if the catalog wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits.cat corresponding to the image wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits.cat corresponding to the image wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits
WCS catalog name: wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=5592, passed=67166
Got 67166 stars (including 61518 good ones) from the SExtractor catalog wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits.cat
util/solve_plate_with_UCAC5 got 67166 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 935 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: 0.65"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.66"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.66"
Estimated accuracy of the plate solution: 0.73"
Excluding outliers - 925 stars left (next iteration limit 1017)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits -region wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.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-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
Saving fully-calibrated image wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_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_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
Saving fully-calibrated image wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-51-54_20.00sec_-15.00C_LIGHT_0375.fits
Saving fully-calibrated image wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_035606_TTUQ2b1x1_11803_Mo0o5pzJ/wcs_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376.fits
Preparing the HTML report for the field Cyg-08-Q2b1x1 with default.sex.telephoto_lens_vSTL
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Adding exclusion_list_gaiadr2.txt__out213610.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294969.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296594.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316812.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316813.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316815.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316821.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316849.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out317586.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out317774.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out49137.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71564.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out110658.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out125660.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136464.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138965.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out184065.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193407.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out220891.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236879.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316817.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316819.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316822.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316830.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316837.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316840.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316843.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316845.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out64490.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out89026.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out90024.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 28s
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: 9s
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Considering the candidate 316812_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 316812_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:55:20.45 +31:25:25.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 1.194 2033621625449848192 298.83519174055 +31.42352967181 12.2846 11.2886 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.194#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 316813_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 316813_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 20:25:27.62 +31:29:03.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 4.015 1862008892823930496 306.36414085346 +31.48513451008 12.3242 11.7739 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.015#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 316815_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 316815_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 20:25:29.48 +29:26:15.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 3.586 1860496583291407104 306.37172282893 +29.43779404292 12.0955 11.6323 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.586#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 316817_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
Preparing report for the candidate 316817_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
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Considering the candidate 316819_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
Preparing report for the candidate 316819_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
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Considering the candidate 316821_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 316821_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 20:25:13.85 +31:31:47.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 4.753 1862021154932287744 306.30807280030 +31.52863333499 12.2498 11.8908 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.753#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 316822_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
Preparing report for the candidate 316822_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
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Considering the candidate 316826_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 316826_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 316830_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
Preparing report for the candidate 316830_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
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Considering the candidate 316837_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
Preparing report for the candidate 316837_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
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Considering the candidate 316840_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
Preparing report for the candidate 316840_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
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Considering the candidate 316843_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
Preparing report for the candidate 316843_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
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Considering the candidate 316845_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
Preparing report for the candidate 316845_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
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Considering the candidate 316849_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 316849_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:54:04.42 +33:48:36.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.63, MAG_FAINT_SEARCH_LIMIT=12.61)GAIADR2_OUTPUT=# 0.286 2035133320828876160 298.51832256276 +33.81004170175 11.6506 11.4051 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.286#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 316976_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 316976_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:30:39.83 +27:54:38.4 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 317225_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 317225_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 317294_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 317294_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:39:39.34 +33:59:11.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 317398_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 317398_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 20:14:18.55 +28:40:28.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 317421_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 317421_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:44:46.86 +29:14:30.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 317437_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 317437_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:30:33.27 +27:57:52.8 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 317439_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 317439_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 20:01:02.50 +27:43:52.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 317452_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 317452_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 20:10:39.13 +26:55:52.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 317473_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 317473_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 317586_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 317586_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:56:39.84 +30:58:07.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.39, MAG_FAINT_SEARCH_LIMIT=13.37)GAIADR2_OUTPUT=# 3.250 2030524820935398784 299.16514851604 +30.96922547968 12.6403 12.1845 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.250#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 317657_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 317657_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 317683_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 317683_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:49:51.20 +27:06:23.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 317712_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 317712_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:49:50.60 +28:27:41.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 317752_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 317752_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 317774_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 317774_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 20:18:25.20 +33:16:14.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.55, MAG_FAINT_SEARCH_LIMIT=13.53)GAIADR2_OUTPUT=# 2.395 2054608725437796736 304.60487880725 +33.27137976394 12.7637 12.3293 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.395#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 317789_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 317789_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 317807_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 317807_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 317834_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 317834_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 317866_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 317866_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 88157_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 88157_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:30:44.21 +27:57:41.6 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 200523_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 200523_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 20:23:51.62 +32:11:23.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 236436_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 236436_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:46:25.77 +33:43:27.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 188289_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 188289_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 90024_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
Preparing report for the candidate 90024_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
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Considering the candidate 89026_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
Preparing report for the candidate 89026_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
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Considering the candidate 295891_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 295891_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 20:27:55.55 +30:59:23.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 296594_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 296594_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 20:26:27.47 +28:54:24.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 2.825 1860416456379568256 306.61532676048 +28.90666632850 11.8016 11.4550 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.825#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 111422_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 111422_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:55:45.73 +29:24:32.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236879_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
Preparing report for the candidate 236879_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
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Considering the candidate 49137_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 49137_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:51:01.69 +27:04:26.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)
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Considering the candidate 136464_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
Preparing report for the candidate 136464_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
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Considering the candidate 110658_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
Preparing report for the candidate 110658_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
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Considering the candidate 213610_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 213610_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 20:26:17.96 +32:49:38.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)GAIADR2_OUTPUT=# 0.257 2055893268563390720 306.57475577121 +32.82741510067 11.9216 11.3035 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.257#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 64490_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
Preparing report for the candidate 64490_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
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Considering the candidate 71564_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 71564_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 20:26:13.14 +28:11:37.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.33, MAG_FAINT_SEARCH_LIMIT=13.31)GAIADR2_OUTPUT=# 1.124 1860099316000691072 306.55507494186 +28.19373536939 12.0663 11.5469 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.124#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193407_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
Preparing report for the candidate 193407_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
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Considering the candidate 73692_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 73692_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:49:26.69 +28:05:03.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 125660_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
Preparing report for the candidate 125660_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
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Considering the candidate 220891_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
Preparing report for the candidate 220891_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
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Considering the candidate 294969_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 294969_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 20:21:52.36 +30:01:45.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.93, MAG_FAINT_SEARCH_LIMIT=12.91)
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Considering the candidate 50933_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 50933_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236091_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 236091_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:57:07.34 +33:51:25.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 184065_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
Preparing report for the candidate 184065_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
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Considering the candidate 138965_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
Preparing report for the candidate 138965_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
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Considering the candidate 60196_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 60196_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:51:30.92 +27:27:36.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 157240_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 157240_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:57:08.34 +30:46:39.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 163012_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 163012_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:56:41.70 +30:56:51.3 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 155703_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 155703_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:55:05.31 +30:41:15.7 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 76527_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 76527_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:53:16.00 +28:05:59.2 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171896_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 171896_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 20:00:58.76 +31:13:49.8 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130012_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 130012_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 20:03:43.51 +29:59:22.1 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 91477_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 91477_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:57:23.68 +28:41:38.2 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 166655_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 166655_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 20:01:55.58 +31:07:03.8 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 188794_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 188794_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:59:39.16 +31:49:36.6 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58980_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 58980_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:59:09.12 +27:30:46.2 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 139496_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 139496_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:55:06.56 +30:11:42.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 127342_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 127342_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 20:03:38.81 +29:53:35.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39399_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 39399_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:53:52.67 +26:35:36.0 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 165195_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 165195_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:58:38.15 +30:59:02.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 80281_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 80281_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:52:15.72 +28:15:06.0 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192265_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 192265_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 20:02:48.79 +31:57:29.9 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86896_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 86896_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:49:54.76 +28:26:23.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 65096_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 65096_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 20:01:06.23 +27:45:16.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200287_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 200287_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 20:04:36.13 +32:13:04.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116971_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 116971_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:42:49.26 +29:19:56.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52282_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 52282_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:49:55.87 +27:05:07.4 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29945_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 29945_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 20:00:15.38 +26:11:16.5 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 223982_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 223982_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:46:35.06 +32:53:16.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102040_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 102040_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 20:17:31.48 +29:08:52.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 89079_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 89079_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 20:14:14.45 +28:41:42.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160852_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 160852_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:43:09.68 +30:40:41.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 238601_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 238601_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:48:50.64 +33:26:14.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 44319_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 44319_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 20:10:33.52 +26:54:17.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 65977_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 65977_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 20:15:45.87 +27:48:53.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 41894_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 41894_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 20:11:47.94 +26:48:33.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 55567_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 55567_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:43:56.04 +27:08:08.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 120334_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 120334_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:37:09.62 +29:20:01.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34195_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 34195_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 20:12:00.67 +26:28:44.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 212460_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 212460_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:42:44.70 +32:25:37.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 147684_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 147684_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:39:22.91 +30:09:13.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170384_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 170384_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 20:22:37.23 +31:15:53.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 241308_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 241308_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 20:15:23.71 +33:43:41.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255388_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 255388_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:34:56.43 +33:47:42.5 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 275957_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 275957_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:39:44.94 +33:58:45.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 48596_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 48596_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:31:21.78 +26:37:03.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25990_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 25990_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:43:43.04 +25:46:20.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 126219_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376
The candidate 126219_fd_Cyg-08-Q2b1x1_2026-03-27_03-52-37_20.00sec_-15.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:34:51.11 +29:27:48.7 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 5s
make_report_in_HTML.sh TOTAL: 42s
Prepared the HTML report for the field Cyg-08-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
19:52:10.20 +29:21:06.2
20:25:48.67 +29:58:52.2
20:27:04.64 +30:17:21.1
20:27:49.84 +30:21:40.0
20:27:51.49 +31:48:04.7
20:25:07.40 +32:06:59.2
20:27:39.35 +33:04:48.1
19:49:13.77 +33:44:55.9
19:40:01.06 +32:06:52.4
19:55:44.73 +32:19:10.4
20:24:38.89 +29:13:54.1
19:56:31.72 +33:53:49.6
19:29:34.95 +28:21:45.6
20:25:47.57 +28:39:01.0
19:32:24.89 +31:14:26.8
19:33:33.79 +28:51:50.3
19:50:12.84 +27:43:33.5
19:35:01.07 +28:22:16.8
19:33:52.27 +28:19:44.3
########### Completed Cyg-08-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 ####
19:40:01.06 +32:06:52.4
19:55:44.73 +32:19:10.4
20:24:38.89 +29:13:54.1
19:56:31.72 +33:53:49.6
19:29:34.95 +28:21:45.6
20:25:47.57 +28:39:01.0
19:32:24.89 +31:14:26.8
19:33:33.79 +28:51:50.3
19:33:52.27 +28:19:44.3
19:35:01.07 +28:22:16.8
19:49:13.77 +33:44:55.9
20:27:04.64 +30:17:21.1
19:52:10.20 +29:21:06.2
19:50:12.84 +27:43:33.5
20:25:07.40 +32:06:59.2
20:25:48.67 +29:58:52.2
20:27:39.35 +33:04:48.1
20:27:51.49 +31:48:04.7
20:27:49.84 +30:21:40.0
###################################################################################
19:40:01.06 +32:06:52.4 -- not an asteroid (will add it to exclusion list)
19:55:44.73 +32:19:10.4 -- not an asteroid (will add it to exclusion list)
20:24:38.89 +29:13:54.1 -- not an asteroid (will add it to exclusion list)
19:56:31.72 +33:53:49.6 -- not an asteroid (will add it to exclusion list)
19:29:34.95 +28:21:45.6 -- not an asteroid (will add it to exclusion list)
20:25:47.57 +28:39:01.0 -- not an asteroid (will add it to exclusion list)
19:32:24.89 +31:14:26.8 -- not an asteroid (will add it to exclusion list)
19:33:33.79 +28:51:50.3 -- not an asteroid (will add it to exclusion list)
19:33:52.27 +28:19:44.3 -- not an asteroid (will add it to exclusion list)
19:35:01.07 +28:22:16.8 -- not an asteroid (will add it to exclusion list)
19:49:13.77 +33:44:55.9 -- not an asteroid (will add it to exclusion list)
20:27:04.64 +30:17:21.1 -- not an asteroid (will add it to exclusion list)
19:52:10.20 +29:21:06.2 -- not an asteroid (will add it to exclusion list)
19:50:12.84 +27:43:33.5 -- not an asteroid (will add it to exclusion list)
20:25:07.40 +32:06:59.2 -- not an asteroid (will add it to exclusion list)
20:25:48.67 +29:58:52.2 -- not an asteroid (will add it to exclusion list)
20:27:39.35 +33:04:48.1 -- not an asteroid (will add it to exclusion list)
20:27:51.49 +31:48:04.7 -- not an asteroid (will add it to exclusion list)
20:27:49.84 +30:21:40.0 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
19:29:34.95 +28:21:45.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:32:24.89 +31:14:26.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:33:33.79 +28:51:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:33:52.27 +28:19:44.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:35:01.07 +28:22:16.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:40:01.06 +32:06:52.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:49:13.77 +33:44:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:50:12.84 +27:43:33.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:52:10.20 +29:21:06.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:55:44.73 +32:19:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:56:31.72 +33:53:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:24:38.89 +29:13:54.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:25:07.40 +32:06:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:25:47.57 +28:39:01.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:25:48.67 +29:58:52.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:27:04.64 +30:17:21.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:27:39.35 +33:04:48.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:27:49.84 +30:21:40.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:27:51.49 +31:48:04.7 -- 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)
19:29:34.95 +28:21:45.6 -- not a known variable star
19:32:24.89 +31:14:26.8 -- a known variable star
19:33:33.79 +28:51:50.3 -- not a known variable star
19:33:52.27 +28:19:44.3 -- a known variable star
19:35:01.07 +28:22:16.8 -- a known variable star
19:40:01.06 +32:06:52.4 -- not a known variable star
19:49:13.77 +33:44:55.9 -- not a known variable star
19:50:12.84 +27:43:33.5 -- a known variable star
19:52:10.20 +29:21:06.2 -- a known variable star
19:55:44.73 +32:19:10.4 -- a known variable star
19:56:31.72 +33:53:49.6 -- a known variable star
20:24:38.89 +29:13:54.1 -- not a known variable star
20:25:07.40 +32:06:59.2 -- not a known variable star
20:25:47.57 +28:39:01.0 -- a known variable star
20:25:48.67 +29:58:52.2 -- not a known variable star
20:27:04.64 +30:17:21.1 -- not a known variable star
20:27:39.35 +33:04:48.1 -- not a known variable star
20:27:49.84 +30:21:40.0 -- not a known variable star
20:27:51.49 +31:48:04.7 -- not a known variable star
Found 11 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
19 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
###################################################################################
Adding identified Gaia sources from exclusion_list_gaiadr2.txt
exclusion_list_apass.txt NOT FOUND
IS_THIS_TEST_RUN= NO ALLOW_EXCLUSION_LIST_UPDATE= YES
#### Adding the following to the exclusion list ####
19:29:34.95 +28:21:45.6
19:32:24.89 +31:14:26.8
19:33:33.79 +28:51:50.3
19:33:52.27 +28:19:44.3
19:35:01.07 +28:22:16.8
19:40:01.06 +32:06:52.4
19:49:13.77 +33:44:55.9
19:50:12.84 +27:43:33.5
19:52:10.20 +29:21:06.2
19:55:44.73 +32:19:10.4
19:56:31.72 +33:53:49.6
20:24:38.89 +29:13:54.1
20:25:07.40 +32:06:59.2
20:25:47.57 +28:39:01.0
20:25:48.67 +29:58:52.2
20:27:04.64 +30:17:21.1
20:27:39.35 +33:04:48.1
20:27:49.84 +30:21:40.0
20:27:51.49 +31:48:04.7
20:26:17.96 +32:49:38.8
20:21:52.36 +30:01:45.7
20:26:27.47 +28:54:24.7
19:55:20.45 +31:25:25.9
20:25:27.62 +31:29:03.7
20:25:29.48 +29:26:15.2
20:25:13.85 +31:31:47.7
19:54:04.42 +33:48:36.2
19:56:39.84 +30:58:07.3
20:18:25.20 +33:16:14.6
19:51:01.69 +27:04:26.7
20:26:13.14 +28:11:37.0
####################################################
The observatory MPC code is 500
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461126.86950148 -observatory 500
22:47:03.83 -08:14:41.8 Mercury (0.6mag)
01:35:42.96 +09:17:53.5 Venus (-3.9mag)
23:21:40.40 -05:16:42.0 Mars (1.2mag)
07:05:54.70 +22:56:31.1 Jupiter (-2.2mag)
00:20:16.12 -00:07:22.9 Saturn (0.9mag)
03:43:57.22 +19:35:16.5 Uranus (5.8mag)
00:08:10.57 -00:32:19.5 Neptune (7.8mag)
20:32:32.55 -22:53:04.0 Pluto (14.5mag)
07:57:23.67 +24:15:22.1 Moon (-10.9mag)
-rw-r--r-- 1 apache apache 362 Mar 27 04:00 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461126.86950148:
07:05:48.22 +22:56:45.0 Io (5.6mag)
07:05:53.67 +22:56:29.5 Europa (5.8mag)
07:05:43.76 +22:56:44.8 Ganymede (5.2mag)
07:06:10.51 +22:56:11.0 Callisto (6.5mag)
07:09:52.24 +22:54:26.6 Himalia (15.2mag)
07:05:58.56 +22:56:22.5 Thebe (16.1mag)
07:09:35.53 +23:20:18.6 Elara (17.2mag)
07:03:27.85 +23:46:49.7 Pasiphae (17.3mag)
07:14:36.64 +22:52:03.9 Carme (18.4mag)
00:20:27.89 -00:07:20.2 Titan (8.8mag)
00:20:16.39 -00:07:07.7 Rhea (10.1mag)
00:20:37.48 -00:05:11.1 Iapetus (11.5mag)
00:20:17.86 -00:06:59.1 Hyperion (14.8mag)
00:22:06.69 +00:03:21.2 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Mar 27 04:00 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461126.86950148:
13:40:11.84 +01:55:06.6 JWST
18:06:53.17 +32:57:03.9 Chandra
08:46:42.94 -44:41:54.8 XMM-Newton
-rw-r--r-- 1 apache apache 96 Mar 27 04:00 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461126.86950148 -observatory 500
18:40:31.17 -27:45:03.5 14.0mag P/2010 H2 (Vales)
04:54:20.51 -70:40:29.5 17.5mag C/2014 UN271 (Bernardinelli-Bernstein)
05:29:15.28 +31:19:32.6 17.1mag C/2017 K2 (PANSTARRS)
17:30:28.24 +08:10:31.5 17.6mag C/2021 G2 (ATLAS)
23:03:58.38 +28:34:41.5 17.0mag C/2022 E2 (ATLAS)
04:07:11.99 +25:28:45.7 15.8mag C/2022 N2 (PANSTARRS)
09:01:29.87 +31:40:20.9 16.1mag C/2022 QE78 (ATLAS)
08:29:48.82 -02:23:32.2 17.2mag C/2022 R6 (PANSTARRS)
18:56:27.14 +16:50:29.5 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:45:31.89 -11:46:53.2 17.6mag P/2023 B1 (PANSTARRS)
09:19:28.51 -15:12:18.4 17.5mag C/2023 F3 (ATLAS)
21:30:51.35 +61:55:46.1 17.4mag C/2023 H5 (Lemmon)
19:31:11.92 -03:32:38.1 14.4mag C/2023 R1 (PANSTARRS)
21:40:51.90 +83:28:46.6 17.7mag C/2023 X2 (Lemmon)
06:14:00.37 +63:41:59.6 16.9mag C/2024 A1 (ATLAS)
04:25:33.20 +09:28:31.5 9.6mag C/2024 E1 (Wierzchos)
11:17:27.70 +03:58:30.6 18.0mag C/2024 G2 (ATLAS)
16:29:49.84 +03:10:39.7 17.4mag C/2024 G6 (ATLAS)
20:13:16.87 +10:15:09.2 14.8mag C/2024 J3 (ATLAS)
03:09:39.34 -25:33:10.1 16.4mag C/2024 T5 (ATLAS)
05:01:33.15 +50:38:16.1 17.6mag C/2025 J1 (Borisov)
14:54:48.67 +25:56:43.7 14.5mag C/2025 L1 (ATLAS)
02:56:42.86 -23:24:18.8 17.7mag C/2025 Q3 (ATLAS)
22:37:56.11 +19:26:25.5 11.6mag C/2025 R3 (PANSTARRS)
13:02:33.08 +01:44:18.0 17.6mag C/2025 Y1 (ATLAS)
01:51:07.13 -02:14:43.1 12.4mag C/2026 A1 (MAPS)
22:59:57.79 +32:51:09.0 13.9mag C/2026 B2 (Sun-Gao)
18:04:32.86 -10:37:57.5 13.0mag 10P/Tempel
15:22:42.60 +04:47:19.2 12.3mag 24P/Schaumasse
11:09:23.56 -02:14:04.5 15.6mag 29P/Schwassmann-Wachmann
17:49:41.38 -10:23:42.2 17.5mag 40P/Vaisala
10:42:07.47 -05:54:47.7 16.5mag 43P/Wolf-Harrington
01:18:34.53 +14:03:49.6 17.0mag 47P/Ashbrook-Jackson
06:37:37.35 +41:04:46.5 17.1mag 63P/Wild
23:03:02.86 -13:54:33.3 15.7mag 65P/Gunn
03:13:27.53 +13:55:35.9 15.9mag 76P/West-Kohoutek-Ikemura
00:22:58.90 +04:19:15.0 14.6mag 78P/Gehrels
22:00:25.37 -15:02:52.4 14.5mag 88P/Howell
01:17:04.75 +15:06:42.8 15.2mag 93P/Lovas
04:20:27.56 +31:06:24.4 16.4mag 123P/West-Hartley
08:10:29.69 +47:23:52.2 16.2mag 124P/Mrkos
02:03:35.64 +12:06:34.4 16.4mag 128P/Shoemaker-Holt
02:09:30.12 +11:55:44.0 17.4mag 131P/Mueller
23:48:45.85 +05:40:11.1 12.2mag 141P/Machholz
23:59:02.01 -02:19:08.1 12.3mag 141P-A/Machholz
22:55:41.21 -05:18:28.5 15.3mag 141P-D/Machholz
00:08:00.62 -11:10:22.1 15.4mag 162P/SidingSpring
10:35:20.66 +31:56:04.0 17.6mag 164P/Christensen
06:00:47.56 +24:41:20.9 17.6mag 198P/ODAS
15:24:32.48 -02:29:51.5 17.1mag 210P/Christensen
20:35:26.90 -16:08:23.1 17.2mag 218P/LINEAR
17:05:28.00 -16:05:44.5 16.2mag 235P/LINEAR
04:53:45.25 +32:47:50.1 16.4mag 240P/NEAT
07:31:08.70 -07:31:21.1 17.5mag 242P/Spahr
15:47:58.53 +05:34:50.7 17.6mag 391P/Kowalski
07:28:45.62 +21:12:16.8 17.6mag 450P/LONEOS
05:08:51.28 +46:12:37.9 17.3mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.8K Mar 27 04:00 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.87 -53:16:33.70 ASASSN-26cc 2026-03-20.08 3.93
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.90 -45:55:38.40 ASASSN-26bt 2026-03-19.05 16.24
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.45 +15:42:15.00 SN2026ehe 2026-03-12.11 -0.29
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
11:30:09.67 -47:26:43.70 ASASSN-26bn 2026-03-10.12 15.2
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.48 -37:49:32.80 ASASSN-26bk 2026-03-2.3 13.11
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.29 +19:58:46.30 ASASSN-26be 2026-02-25.56 14.95
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:35.79 -79:28:57.30 ASASSN-26bb 2026-02-24.37 16.2
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
04:55:50.66 -29:52:57.70 SN 2026dpg 2026-02-23.11 15.75
04:21:28.18 -53:22:54.40 AT2026drl 2026-02-21.03 17.31
11:50:37.32 +55:21:13.70 SN 2026dix 2026-02-21.43 16.39
16:21:19.69 -63:47:29.40 ASASSN-26az 2026-02-21.03 17.02
02:45:30.93 -54:17:43.10 SN 2026cju 2026-02-21.04 17.54
01:58:40.68 +47:34:50.10 ASASSN-26av 2026-02-21.09 15.97
18:35:53.01 -42:31:38.90 ASASSN-26aw 2026-02-21.12 15.89
11:40:18.88 -39:45:09.20 ASASSN-26ax 2026-02-21.08 15.73
02:26:23.52 -51:42:29.80 ASASSN-26ay 2026-02-21.04 13.93
08:46:07.66 +01:17:43.90 ASASSN-26ba 2026-02-20.23 15.43
14:15:47.69 -48:05:16.40 SN2026dez 2026-02-19.19 15.93
17:25:53.90 -23:28:31.50 ASASSN-26au 2026-02-18.33 15.82
16:07:59.09 -24:00:10.00 SN2026cmv 2026-02-17.28 16.19
18:15:01.25 -37:43:36.70 ASASSN-26at 2026-02-16.36 15.94
13:01:07.08 -11:25:16.30 AT2026bzh 2026-02-12.45 17.3
10:56:29.81 -07:07:25.30 SN 2026bre 2026-02-12.16 17.15
08:55:43.51 -53:26:11.50 ASASSN-26as 2026-02-12.2 16.54
06:33:50.98 -41:46:25.10 ASASSN-26ar 2026-02-12.04 16.42
12:15:22.43 +23:59:39.60 SN2026bzg 2026-02-11.27 16.32
08:01:10.95 -03:43:14.30 AT2026coj 2026-02-9.25 13.73
12:44:00.18 -57:03:46.80 ASASSN-26aq 2026-02-9.18 16
06:26:33.34 -54:06:39.90 AT2026cih 2026-02-8.06 17.26
23:08:59.40 -88:59:11.60 SN 2026bsu 2026-02-8.03 16.02
01:04:14.94 -62:31:02.30 SN 2026azk 2026-02-8.04 16.41
08:44:55.41 +64:55:09.90 SN 2026anq 2026-02-7.16 17.62
12:37:42.99 +33:26:05.40 SN 2026bnm 2026-02-7.29 16.74
00:12:55.45 +33:21:25.90 SN2026cbh 2026-02-7.09 16.33
08:02:12.64 -04:14:20.90 SN 2026auh 2026-02-7.11 16.64
18:03:52.67 -31:27:26.00 TCP J18035290-3127298 2026-02-7.37 15.76
12:18:03.59 +50:27:10.20 SN 2026bjz 2026-02-7.25 16.48
07:51:51.12 +55:05:27.60 SN 2026ail 2026-02-6.21 16.85
08:10:56.38 +36:49:42.80 AT2026bsa 2026-02-6.29 17.47
04:43:45.47 -15:49:01.00 SN2026azr 2026-02-5.24 16.96
06:14:48.48 -34:20:08.90 ASASSN-26ap 2026-02-5.2 13.77
02:42:33.90 -27:21:02.60 SN 2026aip 2026-02-4.09 15.85
00:43:12.26 +38:35:47.90 AT2026brt 2026-02-3.12 14.92
14:34:27.21 +21:56:59.90 SN2026atb 2026-01-29.32 15.59
13:12:04.11 -60:56:12.40 ASASSN-26ao 2026-01-28.35 15.61
13:00:36.49 -06:28:26.00 SN2026azd 2026-01-28.23 15.69
10:33:50.27 -31:00:53.40 SN 2026ayz 2026-01-25.11 15.3
-rw-r--r-- 1 apache apache 5.8K Mar 27 04:00 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 27 04:00 tocp_transients_list.txt