This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-09-Q1b1x1_023236_TTUQ1b1x1_3652972_3vDyaYLu
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 08 06.3130 2461258.8130 10.49 05:38:55.63 +61:27:37.6
151.05259 15.56191 galactic Cam Second-epoch detections are separated by 0.4" and 7.8 pix
The object was found in VSX 1" NSVS J0538557+612738
Type: L:
# Max. Min./Amp. JD0 Period
9.851 R1 Y 0.510 R1 445.000000000000 M3/4
The object was not found in astcheck.
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:38:55.63 +61:27:37.6: 11.56 +/- 0.01 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:38:55.63 +61:27:37.6: 11.55 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.55 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0538557+612738,2461258.8130,10.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0538557+612738 20260806.3130 10.49CV 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
Mean magnitude and position on the discovery images:
2026 08 06.3130 2461258.8130 10.81 05:33:22.20 +61:37:46.7
150.56515 15.06616 galactic Cam Second-epoch detections are separated by 0.9" and 7.7 pix
The object was found in VSX 0" ASASSN-V J053322.20+613747.0
Type: SR
# Max. Min./Amp. JD0 Period
11.850 V 12.120 V 2458466.08130 48.811134300000
The object was not found in astcheck.
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:33:22.20 +61:37:46.7: 11.89 +/- 0.01 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:33:22.20 +61:37:46.7: 11.89 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.89 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J053322.20+613747.0,2461258.8130,10.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J053322.20+613747.0 20260806.3130 10.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3130 2461258.8130 10.73 05:25:02.32 +59:26:05.8
151.96848 13.06309 galactic Cam Second-epoch detections are separated by 0.8" and 7.5 pix
The object was found in VSX 1" ASASSN-V J052502.41+592605.6
Type: SRS
# Max. Min./Amp. JD0 Period
12.110 V 12.250 V 2458067.12000 26.773000000000
The object was not found in astcheck.
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:25:02.32 +59:26:05.8: 11.99 +/- 0.01 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:25:02.32 +59:26:05.8: 11.99 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.99 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J052502.41+592605.6,2461258.8130,10.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J052502.41+592605.6 20260806.3130 10.73CV 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
Mean magnitude and position on the discovery images:
2026 08 06.3130 2461258.8130 11.36 04:02:14.34 +62:43:48.3
142.92017 7.51969 galactic Cam Second-epoch detections are separated by 0.6" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 475039742473271040 | 04:02:14.35 +62:43:49.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.922+/-0.028 (M)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 04:02:14.34 +62:43:48.3: 12.34 +/- 0.01 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 04:02:14.34 +62:43:48.3: 12.30 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.32 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 475039742473271040,2461258.8130,11.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 475039742473271040 20260806.3130 11.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3130 2461258.8130 11.46 05:13:10.70 +57:30:22.5
152.74997 10.71003 galactic Cam Second-epoch detections are separated by 3.6" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J078.2927+57.5055 | 05:13:10.26 +57:30:19.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:13:10.70 +57:30:22.5: 12.39 +/- 0.01 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:13:10.70 +57:30:22.5: 12.35 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.37 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J078.2927+57.5055,2461258.8130,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J078.2927+57.5055 20260806.3130 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3130 2461258.8130 11.29 05:25:41.62 +59:44:54.0
151.73957 13.29848 galactic Cam Second-epoch detections are separated by 1.0" and 7.8 pix
The object was found in VSX 0" ASASSN-V J052541.61+594453.8
Type: SRS
# Max. Min./Amp. JD0 Period
12.640 V 12.730 V 2456984.97000 23.748000000000
The object was not found in astcheck.
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:25:41.62 +59:44:54.0: 12.40 +/- 0.01 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:25:41.62 +59:44:54.0: 12.43 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.42 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J052541.61+594453.8,2461258.8130,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J052541.61+594453.8 20260806.3130 11.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3130 2461258.8130 11.52 04:02:17.59 +62:46:21.5
142.89634 7.55563 galactic Cam Second-epoch detections are separated by 0.6" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 475040051710881024 | 04:02:17.54 +62:46:21.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.279+/-0.030 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 04:02:17.59 +62:46:21.5: 12.45 +/- 0.01 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 04:02:17.59 +62:46:21.5: 12.46 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.46 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 475040051710881024,2461258.8130,11.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 475040051710881024 20260806.3130 11.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3130 2461258.8130 11.55 04:25:53.05 +64:32:55.6
143.54245 10.65128 galactic Cam Second-epoch detections are separated by 2.5" and 7.0 pix
The object was found in VSX 1" ASASSN-V J042553.00+643256.9
Type: L
# Max. Min./Amp. JD0 Period
13.320 V 13.520 V
The object was not found in astcheck.
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 04:25:53.05 +64:32:55.6: 12.53 +/- 0.01 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 04:25:53.05 +64:32:55.6: 12.50 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.52 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J042553.00+643256.9,2461258.8130,11.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J042553.00+643256.9 20260806.3130 11.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3130 2461258.8130 11.59 05:32:23.46 +60:58:24.7
151.09324 14.63752 galactic Cam Second-epoch detections are separated by 1.4" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 283005398114540672 | 05:32:23.55 +60:58:25.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.805+/-0.031 (K)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:32:23.46 +60:58:24.7: 12.55 +/- 0.01 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:32:23.46 +60:58:24.7: 12.56 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.55 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 283005398114540672,2461258.8130,11.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 283005398114540672 20260806.3130 11.59CV 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
Mean magnitude and position on the discovery images:
2026 08 06.3130 2461258.8130 11.63 04:03:00.53 +63:28:10.4
142.48906 8.12960 galactic Cam Second-epoch detections are separated by 2.1" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 476622042784123776 | 04:03:00.49 +63:28:10.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.342+/-0.029 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 04:03:00.53 +63:28:10.4: 12.60 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 04:03:00.53 +63:28:10.4: 12.59 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.59 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 476622042784123776,2461258.8130,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 476622042784123776 20260806.3130 11.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3130 2461258.8130 11.46 05:12:10.10 +57:29:30.2
152.68368 10.59014 galactic Cam Second-epoch detections are separated by 0.9" and 7.7 pix
The object was found in VSX 1" ASASSN-V J051210.22+572929.3
Type: SR
# Max. Min./Amp. JD0 Period
13.820 g Y 0.120 g 2459292.75300 151.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:12:10.10 +57:29:30.2: 12.61 +/- 0.01 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:12:10.10 +57:29:30.2: 12.60 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J051210.22+572929.3,2461258.8130,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J051210.22+572929.3 20260806.3130 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3130 2461258.8130 11.61 05:31:45.06 +60:52:54.3
151.13496 14.52422 galactic Cam Second-epoch detections are separated by 1.4" and 7.9 pix
The object was found in VSX 0" ASASSN-V J053145.06+605254.5
Type: SRS
# Max. Min./Amp. JD0 Period
12.890 V 13.000 V 2458431.99000 23.899000000000
The object was not found in astcheck.
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:31:45.06 +60:52:54.3: 12.61 +/- 0.01 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:31:45.06 +60:52:54.3: 12.60 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J053145.06+605254.5,2461258.8130,11.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J053145.06+605254.5 20260806.3130 11.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3130 2461258.8130 11.64 05:17:23.98 +59:04:48.3
151.73515 12.04969 galactic Cam Second-epoch detections are separated by 0.5" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 281338877788908672 | 05:17:24.04 +59:04:47.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.205+/-0.038 (M)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:17:23.98 +59:04:48.3: 12.64 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:17:23.98 +59:04:48.3: 12.61 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 281338877788908672,2461258.8130,11.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 281338877788908672 20260806.3130 11.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3130 2461258.8130 11.68 03:59:56.49 +64:34:11.7
141.49699 8.73006 galactic Cam Second-epoch detections are separated by 1.0" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 488933755516711552 | 03:59:56.68 +64:34:11.6 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.510+/-0.033 (K)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 03:59:56.49 +64:34:11.7: 12.67 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 03:59:56.49 +64:34:11.7: 12.73 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.69 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 488933755516711552,2461258.8130,11.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 488933755516711552 20260806.3130 11.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3130 2461258.8130 11.84 05:34:18.58 +61:23:55.3
150.83040 15.04941 galactic Cam Second-epoch detections are separated by 0.6" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 286122513580366720 | 05:34:18.50 +61:23:55.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.747+/-0.030 (K)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:34:18.58 +61:23:55.3: 12.78 +/- 0.01 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:34:18.58 +61:23:55.3: 12.77 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 286122513580366720,2461258.8130,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 286122513580366720 20260806.3130 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3130 2461258.8130 11.85 05:31:58.29 +60:29:28.1
151.49755 14.35098 galactic Cam Second-epoch detections are separated by 2.2" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 282933311384439296 | 05:31:58.22 +60:29:27.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.916+/-0.030 (M)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:31:58.29 +60:29:28.1: 12.79 +/- 0.01 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:31:58.29 +60:29:28.1: 12.81 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 282933311384439296,2461258.8130,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 282933311384439296 20260806.3130 11.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3130 2461258.8130 11.53 05:16:44.15 +58:21:23.9
152.30233 11.57790 galactic Cam Second-epoch detections are separated by 1.2" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J079.1647+58.3523 | 05:16:44.20 +58:21:23.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: M4 (LAMOST DR5) J-Ks=1.339+/-0.031 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:16:44.15 +58:21:23.9: 12.84 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:16:44.15 +58:21:23.9: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J079.1647+58.3523,2461258.8130,11.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J079.1647+58.3523 20260806.3130 11.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3130 2461258.8130 11.86 05:27:18.39 +57:34:43.0
153.74571 12.33659 galactic Cam Second-epoch detections are separated by 3.2" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 281480577349856640 | 05:27:18.31 +57:34:42.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.194+/-0.044 (M)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:27:18.39 +57:34:43.0: 12.89 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:27:18.39 +57:34:43.0: 12.86 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.87 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 281480577349856640,2461258.8130,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 281480577349856640 20260806.3130 11.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3130 2461258.8130 11.90 05:20:45.19 +59:10:52.5
151.88876 12.46530 galactic Cam Second-epoch detections are separated by 2.8" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 281156702454713728 | 05:20:45.27 +59:10:53.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.830+/-0.034 (M)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:20:45.19 +59:10:52.5: 12.93 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:20:45.19 +59:10:52.5: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 281156702454713728,2461258.8130,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 281156702454713728 20260806.3130 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3130 2461258.8130 11.63 05:20:41.53 +58:47:16.6
152.22287 12.24569 galactic Cam Second-epoch detections are separated by 0.6" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 281086127553744000 | 05:20:41.70 +58:47:25.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: M3.5V 1995AJ....110.1838R LHS 1757
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:20:41.53 +58:47:16.6: 12.90 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:20:41.53 +58:47:16.6: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 281086127553744000,2461258.8130,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 281086127553744000 20260806.3130 11.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3130 2461258.8130 11.94 05:24:42.31 +60:06:59.4
151.35079 13.38669 galactic Cam Second-epoch detections are separated by 1.1" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 282953136952818304 | 05:24:42.29 +60:06:59.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.977+/-0.032 (M)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:24:42.31 +60:06:59.4: 12.91 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:24:42.31 +60:06:59.4: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 282953136952818304,2461258.8130,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 282953136952818304 20260806.3130 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3130 2461258.8130 11.88 05:24:24.61 +62:37:45.6
149.12428 14.67114 galactic Cam Second-epoch detections are separated by 0.9" and 7.5 pix
The object was found in VSX 1" ASASSN-V J052424.68+623744.3
Type: SR
# Max. Min./Amp. JD0 Period
12.960 V 13.350 V 2457385.00000 721.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:24:24.61 +62:37:45.6: 12.98 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:24:24.61 +62:37:45.6: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J052424.68+623744.3,2461258.8130,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J052424.68+623744.3 20260806.3130 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3130 2461258.8130 11.95 05:33:37.69 +63:19:21.7
149.05063 15.92485 galactic Cam Second-epoch detections are separated by 0.9" and 7.7 pix
The object was found in VSX 2" ASASSN-V J053337.91+631922.5
Type: SR
# Max. Min./Amp. JD0 Period
13.610 V 14.190 V 2457021.70000 107.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:33:37.69 +63:19:21.7: 13.11 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:33:37.69 +63:19:21.7: 13.17 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J053337.91+631922.5,2461258.8130,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J053337.91+631922.5 20260806.3130 11.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3130 2461258.8130 12.31 05:36:55.58 +60:53:52.4
151.44267 15.07914 galactic Cam Second-epoch detections are separated by 1.0" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:36:55.58 +60:53:52.4 (user input) | T | P | (position from user input) J-Ks=1.143+/-0.030 (M)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:36:55.58 +60:53:52.4: 13.51 +/- 0.03 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:36:55.58 +60:53:52.4: 13.54 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.53 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.8130,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.3130 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
Mean magnitude and position on the discovery images:
2026 08 06.3130 2461258.8130 12.10 05:15:23.63 +58:19:51.5
152.22406 11.41734 galactic Cam Second-epoch detections are separated by 2.1" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J078.8483+58.3308 | 05:15:23.60 +58:19:51.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.255+/-0.029 (M)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:15:23.63 +58:19:51.5: 13.26 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:15:23.63 +58:19:51.5: 13.24 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.25 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J078.8483+58.3308,2461258.8130,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J078.8483+58.3308 20260806.3130 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
Mean magnitude and position on the discovery images:
2026 08 06.3130 2461258.8130 12.11 05:30:55.18 +60:37:14.4
151.31479 14.30480 galactic Cam Second-epoch detections are separated by 3.8" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 282949632259246592 | 05:30:55.35 +60:37:14.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.157+/-0.031 (M)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:30:55.18 +60:37:14.4: 13.25 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:30:55.18 +60:37:14.4: 13.30 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 282949632259246592,2461258.8130,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 282949632259246592 20260806.3130 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3130 2461258.8130 11.98 05:16:10.93 +57:59:19.4
152.57293 11.31266 galactic Cam Second-epoch detections are separated by 3.1" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 280950406585812224 | 05:16:10.83 +57:59:19.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K5 (LAMOST DR5) J-Ks=1.208+/-0.027 (M)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:16:10.93 +57:59:19.4: 13.25 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:16:10.93 +57:59:19.4: 13.30 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 280950406585812224,2461258.8130,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 280950406585812224 20260806.3130 11.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3130 2461258.8130 12.10 05:31:48.36 +60:08:44.4
151.79468 14.15905 galactic Cam Second-epoch detections are separated by 1.1" and 7.8 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 282733475145516544 | 05:31:48.23 +60:08:44.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.057+/-0.030 (M)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:31:48.36 +60:08:44.4: 13.10 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:31:48.36 +60:08:44.4: 13.12 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 282733475145516544,2461258.8130,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 282733475145516544 20260806.3130 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
Mean magnitude and position on the discovery images:
2026 08 06.3130 2461258.8130 12.10 05:41:43.20 +63:49:54.5
149.02865 16.95876 galactic Cam Second-epoch detections are separated by 1.7" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:41:43.20 +63:49:54.5 (user input) | T | P | (position from user input) J-Ks=0.856+/-0.034 (M)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:41:43.20 +63:49:54.5: 13.11 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:41:43.20 +63:49:54.5: 13.09 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.8130,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.3130 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
Mean magnitude and position on the discovery images:
2026 08 06.3130 2461258.8130 12.04 05:30:04.50 +59:48:06.6
151.98637 13.79779 galactic Cam Second-epoch detections are separated by 3.6" and 7.8 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 282707464823641088 | 05:30:04.58 +59:48:07.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K7 (LAMOST DR5) J-Ks=1.191+/-0.028 (M)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:30:04.50 +59:48:06.6: 13.09 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:30:04.50 +59:48:06.6: 13.11 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 282707464823641088,2461258.8130,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 282707464823641088 20260806.3130 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
Mean magnitude and position on the discovery images:
2026 08 06.3130 2461258.8130 11.89 05:24:37.77 +57:14:43.8
153.83888 11.85432 galactic Cam Second-epoch detections are separated by 1.4" and 7.9 pix
The object was found in VSX 1" ASASSN-V J052437.68+571442.7
Type: SRS
# Max. Min./Amp. JD0 Period
13.330 V 13.410 V 2457701.90000 13.056000000000
The object was not found in astcheck.
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:24:37.77 +57:14:43.8: 12.98 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:24:37.77 +57:14:43.8: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J052437.68+571442.7,2461258.8130,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J052437.68+571442.7 20260806.3130 11.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3130 2461258.8130 11.87 05:17:31.83 +57:49:59.7
152.80624 11.37520 galactic Cam Second-epoch detections are separated by 2.2" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 280189651915474560 | 05:17:31.96 +57:49:59.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K4 (LAMOST DR5) J-Ks=1.077+/-0.027 (M)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:17:31.83 +57:49:59.7: 12.99 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:17:31.83 +57:49:59.7: 12.96 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 280189651915474560,2461258.8130,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 280189651915474560 20260806.3130 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3130 2461258.8130 11.89 05:29:10.96 +60:36:41.9
151.21095 14.11680 galactic Cam Second-epoch detections are separated by 2.5" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 282992989951777024 | 05:29:11.01 +60:36:43.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.044+/-0.032 (M)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:29:10.96 +60:36:41.9: 12.96 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:29:10.96 +60:36:41.9: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 282992989951777024,2461258.8130,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 282992989951777024 20260806.3130 11.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3130 2461258.8130 11.78 04:01:03.27 +63:13:15.3
142.49033 7.79815 galactic Cam Second-epoch detections are separated by 3.2" and 6.5 pix
The object was found in VSX 2" ASASSN-V J040102.93+631314.9
Type: SRS
# Max. Min./Amp. JD0 Period
14.520 g Y 0.220 g 2459486.90800 28.322000000000
The object was not found in astcheck.
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 04:01:03.27 +63:13:15.3: 12.93 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 04:01:03.27 +63:13:15.3: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J040102.93+631314.9,2461258.8130,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J040102.93+631314.9 20260806.3130 11.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3130 2461258.8130 11.93 05:17:24.51 +57:39:29.5
152.94565 11.26464 galactic Cam Second-epoch detections are separated by 1.1" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 280182539450024448 | 05:17:24.46 +57:39:29.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.984+/-0.027 (M)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:17:24.51 +57:39:29.5: 12.93 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:17:24.51 +57:39:29.5: 12.91 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 280182539450024448,2461258.8130,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 280182539450024448 20260806.3130 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3130 2461258.8130 11.97 05:30:17.92 +60:13:29.3
151.62636 14.03774 galactic Cam Second-epoch detections are separated by 1.0" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 282920185964393088 | 05:30:17.93 +60:13:28.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.794+/-0.033 (K)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:30:17.92 +60:13:29.3: 12.94 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:30:17.92 +60:13:29.3: 12.95 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 282920185964393088,2461258.8130,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 282920185964393088 20260806.3130 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3130 2461258.8130 11.88 05:20:23.60 +58:15:45.7
152.65215 11.92756 galactic Cam Second-epoch detections are separated by 2.3" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 280306612465808384 | 05:20:23.51 +58:15:46.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.772+/-0.034 (K)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:20:23.60 +58:15:45.7: 12.93 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:20:23.60 +58:15:45.7: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 280306612465808384,2461258.8130,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 280306612465808384 20260806.3130 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3130 2461258.8130 11.75 05:33:25.57 +59:36:24.0
152.38038 14.06323 galactic Cam Second-epoch detections are separated by 1.3" and 7.6 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 J083.3572+59.6064 | 05:33:25.73 +59:36:23.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G1 (LAMOST DR5) J-Ks=1.275+/-0.029 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:33:25.57 +59:36:24.0: 12.90 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:33:25.57 +59:36:24.0: 12.95 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J083.3572+59.6064,2461258.8130,11.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J083.3572+59.6064 20260806.3130 11.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3130 2461258.8130 11.96 05:47:24.44 +62:54:04.0
150.19838 17.10522 galactic Cam Second-epoch detections are separated by 0.7" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 286650206144578048 | 05:47:24.44 +62:54:04.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.887+/-0.027 (M)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:47:24.44 +62:54:04.0: 12.88 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:47:24.44 +62:54:04.0: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 286650206144578048,2461258.8130,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 286650206144578048 20260806.3130 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3130 2461258.8130 11.91 05:11:31.50 +60:06:25.0
150.43985 12.00616 galactic Cam Second-epoch detections are separated by 1.0" and 7.6 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 J077.8795+60.1018 | 05:11:31.56 +60:06:25.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.356+/-0.039 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:11:31.50 +60:06:25.0: 12.87 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:11:31.50 +60:06:25.0: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J077.8795+60.1018,2461258.8130,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J077.8795+60.1018 20260806.3130 11.91CV 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
Mean magnitude and position on the discovery images:
2026 08 06.3130 2461258.8130 11.89 05:12:16.18 +57:24:20.6
152.76347 10.55235 galactic Cam Second-epoch detections are separated by 2.6" and 8.1 pix
The object was not found in VSX
The object was found in ASASSN-V 0" ASASSN-V J051216.14+572420.5
Type: SR
MeanMag 13.21 m Amp. 0.12 m Period 19.0872117 d
The object was not found in astcheck.
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:12:16.18 +57:24:20.6: 12.87 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:12:16.18 +57:24:20.6: 12.85 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461258.8130,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260806.3130 11.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3130 2461258.8130 11.73 05:25:54.62 +59:36:04.4
151.88298 13.24458 galactic Cam Second-epoch detections are separated by 0.8" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 282689803918261376 | 05:25:54.57 +59:36:04.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=1.006+/-0.035 (M)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:25:54.62 +59:36:04.4: 12.84 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:25:54.62 +59:36:04.4: 12.79 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 282689803918261376,2461258.8130,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 282689803918261376 20260806.3130 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
Mean magnitude and position on the discovery images:
2026 08 06.3130 2461258.8130 11.65 05:19:19.08 +58:49:11.1
152.09651 12.11370 galactic Cam Second-epoch detections are separated by 2.5" and 7.2 pix
The object was found in VSX 1" ASASSN-V J051919.12+584910.7
Type: SRS
# Max. Min./Amp. JD0 Period
13.040 V 13.190 V 2457263.06000 27.736000000000
The object was not found in astcheck.
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:19:19.08 +58:49:11.1: 12.80 +/- 0.01 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:19:19.08 +58:49:11.1: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J051919.12+584910.7,2461258.8130,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J051919.12+584910.7 20260806.3130 11.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3130 2461258.8130 11.73 05:11:25.37 +57:58:22.1
152.22378 10.78277 galactic Cam Second-epoch detections are separated by 1.2" and 7.6 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 J077.8561+57.9728 | 05:11:25.48 +57:58:22.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.238+/-0.032 (M)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:11:25.37 +57:58:22.1: 12.76 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:11:25.37 +57:58:22.1: 12.78 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J077.8561+57.9728,2461258.8130,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J077.8561+57.9728 20260806.3130 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
Mean magnitude and position on the discovery images:
2026 08 06.3130 2461258.8130 11.79 05:32:22.89 +60:40:32.8
151.35886 14.48730 galactic Cam Second-epoch detections are separated by 3.1" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 282948154790774016 | 05:32:25.70 +60:40:50.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.827+/-0.029 (M)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:32:22.89 +60:40:32.8: 12.75 +/- 0.01 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:32:22.89 +60:40:32.8: 12.80 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 282948154790774016,2461258.8130,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 282948154790774016 20260806.3130 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3130 2461258.8130 11.72 04:06:25.67 +62:15:49.9
143.59732 7.49710 galactic Cam Second-epoch detections are separated by 0.9" and 6.8 pix
The object was found in VSX 2" ASASSN-V J040625.35+621549.4
Type: SR
# Max. Min./Amp. JD0 Period
13.380 V 13.500 V 2457321.86900 35.850000000000
The object was not found in astcheck.
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 04:06:25.67 +62:15:49.9: 12.76 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 04:06:25.67 +62:15:49.9: 12.74 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.75 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J040625.35+621549.4,2461258.8130,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J040625.35+621549.4 20260806.3130 11.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3130 2461258.8130 11.85 05:31:48.63 +59:43:20.3
152.17144 13.94538 galactic Cam Second-epoch detections are separated by 4.5" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 282662586708350208 | 05:31:48.47 +59:43:21.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.137+/-0.030 (M)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:31:48.63 +59:43:20.3: 12.79 +/- 0.01 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:31:48.63 +59:43:20.3: 12.78 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 282662586708350208,2461258.8130,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 282662586708350208 20260806.3130 11.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3130 2461258.8130 11.73 05:32:25.55 +60:40:50.5
151.35728 14.49446 galactic Cam Second-epoch detections are separated by 1.9" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 282948154790774016 | 05:32:25.70 +60:40:50.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.821+/-0.030 (M)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:32:25.55 +60:40:50.5: 12.73 +/- 0.01 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:32:25.55 +60:40:50.5: 12.72 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.73 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 282948154790774016,2461258.8130,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 282948154790774016 20260806.3130 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
Mean magnitude and position on the discovery images:
2026 08 06.3130 2461258.8130 11.75 05:26:21.42 +60:17:36.9
151.30622 13.65424 galactic Cam Second-epoch detections are separated by 2.4" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 282956740428769664 | 05:26:21.46 +60:17:38.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.858+/-0.029 (M)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:26:21.42 +60:17:36.9: 12.73 +/- 0.01 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:26:21.42 +60:17:36.9: 12.72 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.72 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 282956740428769664,2461258.8130,11.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 282956740428769664 20260806.3130 11.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3130 2461258.8130 11.53 05:29:58.65 +61:00:42.8
150.90662 14.40419 galactic Cam Second-epoch detections are separated by 0.4" and 7.8 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 286016926103129216 | 05:29:58.65 +61:00:42.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.246+/-0.033 (M)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:29:58.65 +61:00:42.8: 12.70 +/- 0.01 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:29:58.65 +61:00:42.8: 12.67 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 286016926103129216,2461258.8130,11.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 286016926103129216 20260806.3130 11.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3130 2461258.8130 11.74 05:36:07.53 +60:03:31.3
152.14963 14.58221 galactic Cam Second-epoch detections are separated by 2.2" and 7.7 pix
The object was found in VSX 0" ASASSN-V J053607.56+600331.5
Type: SR
# Max. Min./Amp. JD0 Period
12.940 V 13.090 V 2457615.12000 31.240000000000
The object was not found in astcheck.
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:36:07.53 +60:03:31.3: 12.66 +/- 0.01 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:36:07.53 +60:03:31.3: 12.64 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J053607.56+600331.5,2461258.8130,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J053607.56+600331.5 20260806.3130 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3130 2461258.8130 11.66 04:22:13.42 +62:59:34.8
144.40115 9.28429 galactic Cam Second-epoch detections are separated by 0.3" and 6.9 pix
The object was found in VSX 1" ASASSN-V J042213.57+625934.7
Type: SR
# Max. Min./Amp. JD0 Period
12.910 V 13.120 V 2457967.00000 344.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 04:22:13.42 +62:59:34.8: 12.62 +/- 0.01 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 04:22:13.42 +62:59:34.8: 12.65 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J042213.57+625934.7,2461258.8130,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J042213.57+625934.7 20260806.3130 11.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3130 2461258.8130 11.66 04:04:20.63 +63:26:50.0
142.61616 8.21274 galactic Cam Second-epoch detections are separated by 0.6" and 6.5 pix
The object was found in VSX 6" Gaia DR3 476619775041343616
Type: ROT
# Max. Min./Amp. JD0 Period
14.940 G 14.980 G M
ATTENTION: measured mag 11.66 is 3.3 mag brighter than the VSX record maximum brightness 14.94 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 04:04:20.63 +63:26:50.0: 12.61 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 04:04:20.63 +63:26:50.0: 12.57 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.59 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 476619775041343616,2461258.8130,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 476619775041343616 20260806.3130 11.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3130 2461258.8130 11.64 04:00:49.34 +64:12:08.8
141.81488 8.51719 galactic Cam Second-epoch detections are separated by 2.1" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 488723233399660672 | 04:00:49.31 +64:12:07.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.473+/-0.033 (K)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 04:00:49.34 +64:12:08.8: 12.53 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 04:00:49.34 +64:12:08.8: 12.58 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.56 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 488723233399660672,2461258.8130,11.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 488723233399660672 20260806.3130 11.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3130 2461258.8130 11.49 04:02:52.89 +62:32:54.0
143.09765 7.43299 galactic Cam Second-epoch detections are separated by 1.4" and 6.7 pix
The object was found in VSX 3" ASASSN-V J040252.57+623252.8
Type: SRS
# Max. Min./Amp. JD0 Period
13.100 V 13.220 V 2458000.00500 22.838000000000
The object was not found in astcheck.
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 04:02:52.89 +62:32:54.0: 12.50 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 04:02:52.89 +62:32:54.0: 12.49 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.49 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J040252.57+623252.8,2461258.8130,11.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J040252.57+623252.8 20260806.3130 11.49CV 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
Mean magnitude and position on the discovery images:
2026 08 06.3130 2461258.8130 11.57 05:25:16.39 +58:59:13.0
152.37516 12.85206 galactic Cam Second-epoch detections are separated by 0.9" and 7.6 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 J081.3177+58.9868 | 05:25:16.26 +58:59:12.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: K5 (LAMOST DR5) J-Ks=1.029+/-0.037 (M)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:25:16.39 +58:59:13.0: 12.50 +/- 0.01 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:25:16.39 +58:59:13.0: 12.54 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.52 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J081.3177+58.9868,2461258.8130,11.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J081.3177+58.9868 20260806.3130 11.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3130 2461258.8130 11.51 05:36:29.67 +60:26:04.3
151.83442 14.80667 galactic Cam Second-epoch detections are separated by 1.5" and 7.9 pix
The object was found in VSX 1" ASASSN-V J053629.72+602603.9
Type: SRS
# Max. Min./Amp. JD0 Period
12.680 V 12.760 V 2458379.02000 27.060000000000
The object was not found in astcheck.
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:36:29.67 +60:26:04.3: 12.49 +/- 0.01 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:36:29.67 +60:26:04.3: 12.52 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.50 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J053629.72+602603.9,2461258.8130,11.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J053629.72+602603.9 20260806.3130 11.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3130 2461258.8130 11.40 05:18:55.15 +58:43:40.0
152.14635 12.02013 galactic Cam Second-epoch detections are separated by 1.4" and 7.6 pix
The object was found in VSX 1" ASASSN-V J051855.04+584338.9
Type: L
# Max. Min./Amp. JD0 Period
12.520 V 12.710 V
The object was not found in astcheck.
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:18:55.15 +58:43:40.0: 12.48 +/- 0.01 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:18:55.15 +58:43:40.0: 12.46 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.47 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J051855.04+584338.9,2461258.8130,11.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J051855.04+584338.9 20260806.3130 11.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3130 2461258.8130 11.46 05:28:38.93 +57:14:48.0
154.13202 12.31625 galactic Cam Second-epoch detections are separated by 1.7" and 8.0 pix
The object was found in VSX 1" ASASSN-V J052839.02+571447.1
Type: SR
# Max. Min./Amp. JD0 Period
12.770 V 12.900 V 2457774.93000 30.630000000000
The object was not found in astcheck.
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:28:38.93 +57:14:48.0: 12.40 +/- 0.01 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:28:38.93 +57:14:48.0: 12.40 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.40 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J052839.02+571447.1,2461258.8130,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J052839.02+571447.1 20260806.3130 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3130 2461258.8130 11.24 05:27:56.83 +61:23:37.2
150.43883 14.38875 galactic Cam Second-epoch detections are separated by 0.9" and 7.8 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 286089871827368704 | 05:27:56.88 +61:23:37.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.282+/-0.039 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:27:56.83 +61:23:37.2: 12.35 +/- 0.01 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:27:56.83 +61:23:37.2: 12.37 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.36 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 286089871827368704,2461258.8130,11.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 286089871827368704 20260806.3130 11.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3130 2461258.8130 11.47 04:13:24.14 +60:25:32.9
145.47796 6.72618 galactic Cam Second-epoch detections are separated by 0.6" and 7.0 pix
The object was found in VSX 1" ASASSN-V J041324.06+602531.9
Type: L:
# Max. Min./Amp. JD0 Period
12.790 V 13.070 V
The object was not found in astcheck.
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 04:13:24.14 +60:25:32.9: 12.30 +/- 0.01 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 04:13:24.14 +60:25:32.9: 12.33 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.32 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J041324.06+602531.9,2461258.8130,11.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J041324.06+602531.9 20260806.3130 11.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3130 2461258.8130 11.30 04:03:08.77 +62:16:12.3
143.30748 7.24577 galactic Cam Second-epoch detections are separated by 2.6" and 6.8 pix
The object was found in VSX 2" ZTF J040308.58+621610.3
Type: SR
# Max. Min./Amp. JD0 Period
14.039 g Y 0.316 g 2458419.13920 197.389342300000
The object was not found in astcheck.
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 04:03:08.77 +62:16:12.3: 12.26 +/- 0.01 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 04:03:08.77 +62:16:12.3: 12.26 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.26 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J040308.58+621610.3,2461258.8130,11.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J040308.58+621610.3 20260806.3130 11.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3130 2461258.8130 11.13 05:52:46.58 +62:41:17.9
150.68018 17.56381 galactic Cam Second-epoch detections are separated by 0.4" and 7.9 pix
The object was found in VSX 1" ASASSN-V J055246.67+624118.2
Type: L
# Max. Min./Amp. JD0 Period
12.320 V 13.340 V
The object was not found in astcheck.
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:52:46.58 +62:41:17.9: 12.17 +/- 0.01 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:52:46.58 +62:41:17.9: 12.18 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.18 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J055246.67+624118.2,2461258.8130,11.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J055246.67+624118.2 20260806.3130 11.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3130 2461258.8130 11.04 05:24:12.11 +57:31:54.1
153.56028 11.95880 galactic Cam Second-epoch detections are separated by 0.5" and 7.8 pix
The object was found in VSX 1" NSVS J0524125+573154
Type: SR
# Max. Min./Amp. JD0 Period
13.530 g Y 0.322 g 2458234.54750 185.576124100000 C
The object was not found in astcheck.
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:24:12.11 +57:31:54.1: 12.01 +/- 0.01 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:24:12.11 +57:31:54.1: 11.99 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.00 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0524125+573154,2461258.8130,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0524125+573154 20260806.3130 11.04CV 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
Mean magnitude and position on the discovery images:
2026 08 06.3130 2461258.8130 11.05 05:10:13.79 +57:18:18.8
152.68707 10.26928 galactic Cam Second-epoch detections are separated by 0.2" and 7.6 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 J077.5576+57.3050 | 05:10:13.84 +57:18:18.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: M2 (LAMOST DR5) J-Ks=1.262+/-0.046 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:10:13.79 +57:18:18.8: 11.99 +/- 0.01 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:10:13.79 +57:18:18.8: 12.01 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.00 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J077.5576+57.3050,2461258.8130,11.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J077.5576+57.3050 20260806.3130 11.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.69737530 09.01.2026 04:44:03.226 /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
First image: 2461049.69737530 09.01.2026 04:44:03.226 /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
Last image: 2461258.81331822 06.08.2026 07:31:00.694 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-09-Q1b1x1_023236_TTUQ1b1x1_3652972_3vDyaYLu/fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.50
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: 3
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
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 17419
Objects passed selection criteria: 17299
Measurements per detected object (mean, median, min, max): 2.2 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.2 2.0 2 4
Average stars detected per image: 10071.8
Average stars matched: 9753.5 (96.8402 %)
Memory usage VmPeak: 242500 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Aug 5 15:05:04 CDT 2026
VaST build number 1.0rc89-189-g49d3cdfd
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-05)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Aug 6 02:34:59 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: 2461049.69737530 09.01.2026 04:44:03.226 /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
First image: 2461049.69737530 09.01.2026 04:44:03.226 /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
Last image: 2461258.81331822 06.08.2026 07:31:00.694 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-09-Q1b1x1_023236_TTUQ1b1x1_3652972_3vDyaYLu/fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 104
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.19
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: 21 seconds
Number of parallel threads: 3
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
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 119725
Objects passed selection criteria: 119340
Measurements per detected object (mean, median, min, max): 2.2 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.2 2.0 2 4
Average stars detected per image: 72166.8
Average stars matched: 69152.8 (95.8236 %)
Memory usage VmPeak: 580160 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Aug 5 15:05:04 CDT 2026
VaST build number 1.0rc89-189-g49d3cdfd
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-05)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Aug 6 02:36:02 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/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-09-Q1b1x1_023236_TTUQ1b1x1_3652972_3vDyaYLu/fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-09-Q1b1x1_023236_TTUQ1b1x1_3652972_3vDyaYLu/fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits
SExtractor catalog cache: saved Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat to cache
SExtractor catalog cache: saved Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.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/Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-09-Q1b1x1_023236_TTUQ1b1x1_3652972_3vDyaYLu/fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-09-Q1b1x1_023236_TTUQ1b1x1_3652972_3vDyaYLu/fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.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: 2461258.81266060
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits exists and is non-empty
Saving wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits to local_wcs_cache/
'wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits' -> 'local_wcs_cache/wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits'
wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits exists and is non-empty
Saving wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits to local_wcs_cache/
'wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits' -> 'local_wcs_cache/wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits'
wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits exists and is non-empty
Saving wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits to local_wcs_cache/
'wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits' -> 'local_wcs_cache/wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits'
wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits exists and is non-empty
Saving wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits to local_wcs_cache/
'wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits' -> 'local_wcs_cache/wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits (1st reference image)
verification OK: wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
Image size: 941.5'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:08:28.129 +61:59:49.31 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits (1st new image)
verification OK: wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits
Image size: 942.6'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:08:21.552 +62:00:56.08 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:08:28.129 +61:59:49.31
Second-epoch image center 05:08:21.552 +62:00:56.08
Angular distance between the image centers 0.0226 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits (2nd new image)
verification OK: wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits
Image size: 942.6'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:08:18.646 +62:00:16.95 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:08:28.129 +61:59:49.31
Second-epoch image center 05:08:18.646 +62:00:16.95
Angular distance between the image centers 0.0201 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 05:08:21.552 +62:00:56.08
Second-epoch second image center 05:08:18.646 +62:00:16.95
Angular distance between the image centers 0.01226 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits &> /tmp/tmp.y0TPUQXKzx
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits &> /tmp/tmp.d8o7JKBY4M
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-09-Q1b1x1_023236_TTUQ1b1x1_3652972_3vDyaYLu/fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits &> /tmp/tmp.8ftdTMdeIs
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-09-Q1b1x1_023236_TTUQ1b1x1_3652972_3vDyaYLu/fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-09-Q1b1x1_023236_TTUQ1b1x1_3652972_3vDyaYLu/fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits &> /tmp/tmp.NPbjccHPn1
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-09-Q1b1x1_023236_TTUQ1b1x1_3652972_3vDyaYLu/fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits
Calibrating the magnitude scale
Found non-empty wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.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_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits and wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
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_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits and wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.wcscat
Found non-empty wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits and wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.wcscat
The reference image (wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits) and catalog (wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.wcscat) found
'wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.wcscat' -> 'wcsmag.cat'
Read 18409 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 57.0210 to 95.6707 deg, Dec +55.2642 to +67.4910 deg
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
Tycho-2 catalog search boundaries: RA 57.0210 to 95.6707 deg, Dec 55.2642 to 67.4910 deg
Loaded 14050 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 8127 out of 8888 total matches.
Matched with Tycho-2 8888 out of 18409 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.954200
a=0.000000 b=1.000000 c=22.954200
From vast_summary.log: estimated ref. image limiting mag.: -7.50
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.45
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.45
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 18409 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 57.0210 to 95.6707 deg, Dec +55.2642 to +67.4910 deg
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
Tycho-2 catalog search boundaries: RA 57.0210 to 95.6707 deg, Dec 55.2642 to 67.4910 deg
Loaded 14050 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 8127 out of 8888 total matches.
Matched with Tycho-2 8888 out of 18409 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
Forced-photometry filter: calibrated wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits -> calib.txt_param_ref_wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits (aperture=6.0)
Read 18487 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 57.0213 to 95.6704 deg, Dec +55.2642 to +67.5028 deg
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
Tycho-2 catalog search boundaries: RA 57.0213 to 95.6704 deg, Dec 55.2642 to 67.5028 deg
Loaded 14060 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 8137 out of 8891 total matches.
Matched with Tycho-2 8891 out of 18487 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
Forced-photometry filter: calibrated wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits -> calib.txt_param_ref_wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits (aperture=6.0)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
2.0 pix Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
3.1 pix fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits
3.0 pix fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits
Limiting magnitude estimates:
15.5 mag. Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
15.5 mag. Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
11.8 mag. fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits
11.9 mag. fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits
All-image limiting magnitude estimate: 11.8 (SNR ) 10.0 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.y0TPUQXKzx (6) ############
Parsing command line arguments...
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_2026-08-06_CI_Cam-09-Q1b1x1_023236_TTUQ1b1x1_3652972_3vDyaYLu/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits' -> 'wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
WCS_IMAGE_NAME=wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
WCS-calibrated image found: wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
Checking if the catalog wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.wcscat corresponding to the image wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits alredy exist and is non-empty...
Catalog wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.wcscat corresponding to the image wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
WCS catalog name: wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1604, bad_region=0, passed=18409
Got 18409 stars (including 16782 good ones) from the SExtractor catalog wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.wcscat
util/solve_plate_with_UCAC5 got 18409 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.5)
Done reading UCAC5 zone files...
Matched 4895 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4884 matched stars entering correct_measured_positions(), 4884 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4884 matched stars entering correct_measured_positions(), 18409 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.5)
Done reading UCAC5 zone files...
Matched 4896 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4885 matched stars entering correct_measured_positions(), 18409 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 4885 matched stars entering correct_measured_positions(), 18409 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 4885 stars left (next iteration limit 5372)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits N_match=4885 sigma_overall_arcsec=0.345 sigma_q1_arcsec=0.450 sigma_q2_arcsec=0.345 sigma_q3_arcsec=0.297 sigma_q4_arcsec=0.292 n_q1=1217 n_q2=1178 n_q3=1234 n_q4=1256 worst_quadrant_to_overall_ratio=1.307
The image catalog is written to wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits -region wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.d8o7JKBY4M (6) ############
Parsing command line arguments...
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_2026-08-06_CI_Cam-09-Q1b1x1_023236_TTUQ1b1x1_3652972_3vDyaYLu/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits' -> 'wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
WCS_IMAGE_NAME=wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
WCS-calibrated image found: wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
Checking if the catalog wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits.wcscat corresponding to the image wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits alredy exist and is non-empty...
Catalog wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits.wcscat corresponding to the image wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
WCS catalog name: wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1596, bad_region=0, passed=18487
Got 18487 stars (including 16865 good ones) from the SExtractor catalog wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits.wcscat
util/solve_plate_with_UCAC5 got 18487 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.5)
Done reading UCAC5 zone files...
Matched 4898 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4888 matched stars entering correct_measured_positions(), 4888 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4888 matched stars entering correct_measured_positions(), 18487 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.5)
Done reading UCAC5 zone files...
Matched 4898 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4887 matched stars entering correct_measured_positions(), 18487 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4887 matched stars entering correct_measured_positions(), 18487 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 4887 stars left (next iteration limit 5376)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits N_match=4887 sigma_overall_arcsec=0.327 sigma_q1_arcsec=0.416 sigma_q2_arcsec=0.327 sigma_q3_arcsec=0.297 sigma_q4_arcsec=0.270 n_q1=1208 n_q2=1174 n_q3=1244 n_q4=1261 worst_quadrant_to_overall_ratio=1.271
The image catalog is written to wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits -region wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.8ftdTMdeIs (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_2026-08-06_CI_Cam-09-Q1b1x1_023236_TTUQ1b1x1_3652972_3vDyaYLu/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-09-Q1b1x1_023236_TTUQ1b1x1_3652972_3vDyaYLu/fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-09-Q1b1x1_023236_TTUQ1b1x1_3652972_3vDyaYLu/fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-09-Q1b1x1_023236_TTUQ1b1x1_3652972_3vDyaYLu/fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-09-Q1b1x1_023236_TTUQ1b1x1_3652972_3vDyaYLu/fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-09-Q1b1x1_023236_TTUQ1b1x1_3652972_3vDyaYLu/fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.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_2026-08-06_CI_Cam-09-Q1b1x1_023236_TTUQ1b1x1_3652972_3vDyaYLu/fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits
WCS_IMAGE_NAME=wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits
WCS-calibrated image found: wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits
Checking if the catalog wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits.wcscat corresponding to the image wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits.wcscat corresponding to the image wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-09-Q1b1x1_023236_TTUQ1b1x1_3652972_3vDyaYLu/fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits
WCS catalog name: wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=77, bad_region=0, passed=1792
Got 1792 stars (including 1712 good ones) from the SExtractor catalog wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits.wcscat
util/solve_plate_with_UCAC5 got 1792 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.6'
Seting catalog search parameters based on the expected field of view 942.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013092 (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 0.010473 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.8 to 67.3)
Done reading UCAC5 zone files...
Matched 1654 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1641 matched stars entering correct_measured_positions(), 1639 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1641 matched stars entering correct_measured_positions(), 1789 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.8 to 67.3)
Done reading UCAC5 zone files...
Matched 1653 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 1641 matched stars entering correct_measured_positions(), 1789 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 1641 matched stars entering correct_measured_positions(), 1789 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 1641 stars left (next iteration limit 1805)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=1641 robust_rms=11.615 arcsec worst_quadrant_rms=13.465 arcsec
SIP_REFIT: SIP order 3 trial: matched=1641 robust_rms=0.481 arcsec worst_quadrant_rms=0.536 arcsec
SIP_REFIT: SIP order 5 trial: matched=1641 robust_rms=0.377 arcsec worst_quadrant_rms=0.448 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=1641 robust_rms_before=0.986 arcsec robust_rms_before_corrected=0.419 arcsec robust_rms_after=0.377 arcsec worst_quadrant_rms_before=0.514 worst_quadrant_rms_after=0.448
verification OK: wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits
verification OK: wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits
Image size: 942.8'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:08:21.614 +62:00:55.17 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 1792 stars ###
'wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Cam-09-Q1b1x1_023236_TTUQ1b1x1_3652972_3vDyaYLu/correct_sextractor_wcs_catalog_usingxy2sky3680579.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 0.986 -> 0.377 arcsec)
WCS_QUALITY_DIAG: file=fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits N_match=1641 sigma_overall_arcsec=0.380 sigma_q1_arcsec=0.444 sigma_q2_arcsec=0.437 sigma_q3_arcsec=0.339 sigma_q4_arcsec=0.347 n_q1=324 n_q2=445 n_q3=412 n_q4=460 worst_quadrant_to_overall_ratio=1.169
The image catalog is written to wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-09-Q1b1x1_023236_TTUQ1b1x1_3652972_3vDyaYLu/fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits -region wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.NPbjccHPn1 (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_2026-08-06_CI_Cam-09-Q1b1x1_023236_TTUQ1b1x1_3652972_3vDyaYLu/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-09-Q1b1x1_023236_TTUQ1b1x1_3652972_3vDyaYLu/fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-09-Q1b1x1_023236_TTUQ1b1x1_3652972_3vDyaYLu/fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-09-Q1b1x1_023236_TTUQ1b1x1_3652972_3vDyaYLu/fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-09-Q1b1x1_023236_TTUQ1b1x1_3652972_3vDyaYLu/fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-09-Q1b1x1_023236_TTUQ1b1x1_3652972_3vDyaYLu/fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.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_2026-08-06_CI_Cam-09-Q1b1x1_023236_TTUQ1b1x1_3652972_3vDyaYLu/fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits
WCS_IMAGE_NAME=wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits
WCS-calibrated image found: wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits
Checking if the catalog wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits.wcscat corresponding to the image wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits.wcscat corresponding to the image wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-09-Q1b1x1_023236_TTUQ1b1x1_3652972_3vDyaYLu/fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits
WCS catalog name: wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=71, bad_region=0, passed=1850
Got 1850 stars (including 1777 good ones) from the SExtractor catalog wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits.wcscat
util/solve_plate_with_UCAC5 got 1850 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.6'
Seting catalog search parameters based on the expected field of view 942.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013092 (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 0.010473 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.8 to 67.3)
Done reading UCAC5 zone files...
Matched 1719 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1707 matched stars entering correct_measured_positions(), 1705 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1707 matched stars entering correct_measured_positions(), 1847 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.8 to 67.3)
Done reading UCAC5 zone files...
Matched 1719 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 1708 matched stars entering correct_measured_positions(), 1847 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 1708 matched stars entering correct_measured_positions(), 1847 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 1708 stars left (next iteration limit 1877)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=1708 robust_rms=10.757 arcsec worst_quadrant_rms=12.263 arcsec
SIP_REFIT: SIP order 3 trial: matched=1708 robust_rms=0.455 arcsec worst_quadrant_rms=0.534 arcsec
SIP_REFIT: SIP order 5 trial: matched=1708 robust_rms=0.374 arcsec worst_quadrant_rms=0.433 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=1708 robust_rms_before=0.977 arcsec robust_rms_before_corrected=0.410 arcsec robust_rms_after=0.374 arcsec worst_quadrant_rms_before=0.537 worst_quadrant_rms_after=0.433
verification OK: wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits
verification OK: wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits
Image size: 942.8'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:08:18.708 +62:00:15.98 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 1850 stars ###
'wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Cam-09-Q1b1x1_023236_TTUQ1b1x1_3652972_3vDyaYLu/correct_sextractor_wcs_catalog_usingxy2sky3680503.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 0.977 -> 0.374 arcsec)
WCS_QUALITY_DIAG: file=fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits N_match=1708 sigma_overall_arcsec=0.405 sigma_q1_arcsec=0.466 sigma_q2_arcsec=0.445 sigma_q3_arcsec=0.353 sigma_q4_arcsec=0.368 n_q1=349 n_q2=446 n_q3=425 n_q4=488 worst_quadrant_to_overall_ratio=1.151
The image catalog is written to wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-09-Q1b1x1_023236_TTUQ1b1x1_3652972_3vDyaYLu/fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits -region wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits sigma_overall=0.345 worst_q_ratio=1.307
ref2=Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits sigma_overall=0.327 worst_q_ratio=1.271
new1=fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits sigma_overall=0.380 worst_q_ratio=1.169
new2=fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits sigma_overall=0.405 worst_q_ratio=1.151
reference average sigma_overall=0.336 worst_q_ratio=1.289
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171_astrometric_residuals.png (4885 matched stars from wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.31 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172_astrometric_residuals.png (4887 matched stars from wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.29 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276_astrometric_residuals.png (1641 matched stars from wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.31 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277_astrometric_residuals.png (1708 matched stars from wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.32 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-09-Q1b1x1_023236_TTUQ1b1x1_3652972_3vDyaYLu/wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits'
Saving fully-calibrated image wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-09-Q1b1x1_023236_TTUQ1b1x1_3652972_3vDyaYLu/wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits'
Preparing the HTML report for the field Cam-09-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Cam-09-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-09-Q1b1x1_023236_TTUQ1b1x1_3652972_3vDyaYLu/fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-09-Q1b1x1_023236_TTUQ1b1x1_3652972_3vDyaYLu/fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits
SExtractor catalog cache: saved Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat to cache
SExtractor catalog cache: saved Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-09-Q1b1x1_023236_TTUQ1b1x1_3652972_3vDyaYLu/fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-09-Q1b1x1_023236_TTUQ1b1x1_3652972_3vDyaYLu/fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
Creating symlink local_wcs_cache/wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
Creating symlink local_wcs_cache/wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits
Creating symlink local_wcs_cache/wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.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_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits exists and is non-empty
wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits exists and is non-empty
wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits exists and is non-empty
wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits (1st reference image)
verification OK: wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
Image size: 941.5'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:08:28.129 +61:59:49.31 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits (1st new image)
verification OK: wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits
Image size: 942.6'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:08:21.552 +62:00:56.08 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:08:28.129 +61:59:49.31
Second-epoch image center 05:08:21.552 +62:00:56.08
Angular distance between the image centers 0.0226 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits (2nd new image)
verification OK: wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits
Image size: 942.6'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:08:18.646 +62:00:16.95 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:08:28.129 +61:59:49.31
Second-epoch image center 05:08:18.646 +62:00:16.95
Angular distance between the image centers 0.0201 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 05:08:21.552 +62:00:56.08
Second-epoch second image center 05:08:18.646 +62:00:16.95
Angular distance between the image centers 0.01226 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits &> /tmp/tmp.K9PzdPeQKt
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits &> /tmp/tmp.uVHYRlN8Y7
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-09-Q1b1x1_023236_TTUQ1b1x1_3652972_3vDyaYLu/fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits &> /tmp/tmp.2QynY3SIM3
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-09-Q1b1x1_023236_TTUQ1b1x1_3652972_3vDyaYLu/fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-09-Q1b1x1_023236_TTUQ1b1x1_3652972_3vDyaYLu/fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits &> /tmp/tmp.qBSFO5eZVS
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-09-Q1b1x1_023236_TTUQ1b1x1_3652972_3vDyaYLu/fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits
Calibrating the magnitude scale
Found non-empty wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.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_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits and wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
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_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits and wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.wcscat
Found non-empty wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits and wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.wcscat
The reference image (wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits) and catalog (wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.wcscat) found
'wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.wcscat' -> 'wcsmag.cat'
Read 131449 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 56.9449 to 95.6878 deg, Dec +55.1944 to +67.5009 deg
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
Tycho-2 catalog search boundaries: RA 56.9449 to 95.6878 deg, Dec 55.1944 to 67.5009 deg
Loaded 14168 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 6814 out of 8995 total matches.
Matched with Tycho-2 8995 out of 131449 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.815000
a=0.000000 b=1.000000 c=22.815000
From vast_summary.log: estimated ref. image limiting mag.: -7.19
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.62
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.62
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 131449 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 56.9449 to 95.6878 deg, Dec +55.1944 to +67.5009 deg
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
Tycho-2 catalog search boundaries: RA 56.9449 to 95.6878 deg, Dec 55.1944 to 67.5009 deg
Loaded 14168 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 6814 out of 8995 total matches.
Matched with Tycho-2 8995 out of 131449 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
Forced-photometry filter: calibrated wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits -> calib.txt_param_ref_wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits (aperture=4.5)
Read 130560 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 56.9451 to 95.7119 deg, Dec +55.1941 to +67.5039 deg
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
Tycho-2 catalog search boundaries: RA 56.9451 to 95.7119 deg, Dec 55.1941 to 67.5039 deg
Loaded 14179 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 6852 out of 9001 total matches.
Matched with Tycho-2 9001 out of 130560 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
Forced-photometry filter: calibrated wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits -> calib.txt_param_ref_wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits (aperture=4.6)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 99 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
1.9 pix Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
1.9 pix Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
2.8 pix fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits
2.8 pix fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits
Limiting magnitude estimates:
15.6 mag. Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
15.6 mag. Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
12.4 mag. fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits
12.4 mag. fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits
All-image limiting magnitude estimate: 12.4 (SNR ) 12.1 (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 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.K9PzdPeQKt (6) ############
Parsing command line arguments...
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_2026-08-06_CI_Cam-09-Q1b1x1_023236_TTUQ1b1x1_3652972_3vDyaYLu/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits' -> 'wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
WCS_IMAGE_NAME=wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
WCS-calibrated image found: wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
Checking if the catalog wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.wcscat corresponding to the image wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits alredy exist and is non-empty...
Catalog wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.wcscat corresponding to the image wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
WCS catalog name: wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=31, blended=12667, bad_region=6, passed=131418
Got 131418 stars (including 118525 good ones) from the SExtractor catalog wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.wcscat
util/solve_plate_with_UCAC5 got 131418 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 725 to 789 (Dec 55.2 to 67.5)
Done reading UCAC5 zone files...
Matched 4903 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4895 matched stars entering correct_measured_positions(), 4895 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4895 matched stars entering correct_measured_positions(), 131418 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 725 to 789 (Dec 55.2 to 67.5)
Done reading UCAC5 zone files...
Matched 4903 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4895 matched stars entering correct_measured_positions(), 131418 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4895 matched stars entering correct_measured_positions(), 131418 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 4895 stars left (next iteration limit 5384)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits N_match=4895 sigma_overall_arcsec=0.316 sigma_q1_arcsec=0.409 sigma_q2_arcsec=0.322 sigma_q3_arcsec=0.286 sigma_q4_arcsec=0.269 n_q1=1174 n_q2=1193 n_q3=1251 n_q4=1277 worst_quadrant_to_overall_ratio=1.296
The image catalog is written to wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits -region wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.uVHYRlN8Y7 (6) ############
Parsing command line arguments...
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_2026-08-06_CI_Cam-09-Q1b1x1_023236_TTUQ1b1x1_3652972_3vDyaYLu/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits' -> 'wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
WCS_IMAGE_NAME=wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
WCS-calibrated image found: wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
Checking if the catalog wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits.wcscat corresponding to the image wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits alredy exist and is non-empty...
Catalog wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits.wcscat corresponding to the image wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
WCS catalog name: wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=33, blended=12449, bad_region=5, passed=130527
Got 130527 stars (including 117842 good ones) from the SExtractor catalog wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits.wcscat
util/solve_plate_with_UCAC5 got 130527 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 725 to 789 (Dec 55.2 to 67.5)
Done reading UCAC5 zone files...
Matched 4906 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4899 matched stars entering correct_measured_positions(), 4899 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4899 matched stars entering correct_measured_positions(), 130527 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 725 to 789 (Dec 55.2 to 67.5)
Done reading UCAC5 zone files...
Matched 4906 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4899 matched stars entering correct_measured_positions(), 130527 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4899 matched stars entering correct_measured_positions(), 130527 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 4899 stars left (next iteration limit 5388)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits N_match=4899 sigma_overall_arcsec=0.314 sigma_q1_arcsec=0.409 sigma_q2_arcsec=0.325 sigma_q3_arcsec=0.268 sigma_q4_arcsec=0.266 n_q1=1189 n_q2=1191 n_q3=1244 n_q4=1275 worst_quadrant_to_overall_ratio=1.302
The image catalog is written to wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits -region wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.2QynY3SIM3 (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_2026-08-06_CI_Cam-09-Q1b1x1_023236_TTUQ1b1x1_3652972_3vDyaYLu/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-09-Q1b1x1_023236_TTUQ1b1x1_3652972_3vDyaYLu/fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-09-Q1b1x1_023236_TTUQ1b1x1_3652972_3vDyaYLu/fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-09-Q1b1x1_023236_TTUQ1b1x1_3652972_3vDyaYLu/fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-09-Q1b1x1_023236_TTUQ1b1x1_3652972_3vDyaYLu/fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-09-Q1b1x1_023236_TTUQ1b1x1_3652972_3vDyaYLu/fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.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_2026-08-06_CI_Cam-09-Q1b1x1_023236_TTUQ1b1x1_3652972_3vDyaYLu/fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits
WCS_IMAGE_NAME=wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits
WCS-calibrated image found: wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits
Checking if the catalog wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits.wcscat corresponding to the image wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits.wcscat corresponding to the image wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-09-Q1b1x1_023236_TTUQ1b1x1_3652972_3vDyaYLu/fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits
WCS catalog name: wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=283, bad_region=2, passed=14082
Got 14082 stars (including 13781 good ones) from the SExtractor catalog wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits.wcscat
util/solve_plate_with_UCAC5 got 14082 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.6'
Seting catalog search parameters based on the expected field of view 942.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013092 (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 0.010473 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.6 to 67.3)
Done reading UCAC5 zone files...
Matched 4875 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4852 matched stars entering correct_measured_positions(), 4853 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4852 matched stars entering correct_measured_positions(), 14082 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.6 to 67.3)
Done reading UCAC5 zone files...
Matched 4875 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4852 matched stars entering correct_measured_positions(), 14082 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Accuracy estimation diagnostic: 4852 matched stars entering correct_measured_positions(), 14082 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 4852 stars left (next iteration limit 5337)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits N_match=4852 sigma_overall_arcsec=0.528 sigma_q1_arcsec=0.637 sigma_q2_arcsec=0.587 sigma_q3_arcsec=0.476 sigma_q4_arcsec=0.469 n_q1=995 n_q2=1166 n_q3=1320 n_q4=1371 worst_quadrant_to_overall_ratio=1.206
The image catalog is written to wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-09-Q1b1x1_023236_TTUQ1b1x1_3652972_3vDyaYLu/fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits -region wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.qBSFO5eZVS (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_2026-08-06_CI_Cam-09-Q1b1x1_023236_TTUQ1b1x1_3652972_3vDyaYLu/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-09-Q1b1x1_023236_TTUQ1b1x1_3652972_3vDyaYLu/fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-09-Q1b1x1_023236_TTUQ1b1x1_3652972_3vDyaYLu/fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-09-Q1b1x1_023236_TTUQ1b1x1_3652972_3vDyaYLu/fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-09-Q1b1x1_023236_TTUQ1b1x1_3652972_3vDyaYLu/fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-09-Q1b1x1_023236_TTUQ1b1x1_3652972_3vDyaYLu/fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.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_2026-08-06_CI_Cam-09-Q1b1x1_023236_TTUQ1b1x1_3652972_3vDyaYLu/fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits
WCS_IMAGE_NAME=wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits
WCS-calibrated image found: wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits
Checking if the catalog wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits.wcscat corresponding to the image wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits.wcscat corresponding to the image wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-09-Q1b1x1_023236_TTUQ1b1x1_3652972_3vDyaYLu/fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits
WCS catalog name: wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=303, bad_region=2, passed=14576
Got 14576 stars (including 14254 good ones) from the SExtractor catalog wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits.wcscat
util/solve_plate_with_UCAC5 got 14576 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.6'
Seting catalog search parameters based on the expected field of view 942.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013092 (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 0.010473 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.6 to 67.3)
Done reading UCAC5 zone files...
Matched 4877 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4855 matched stars entering correct_measured_positions(), 4855 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4855 matched stars entering correct_measured_positions(), 14576 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.6 to 67.3)
Done reading UCAC5 zone files...
Matched 4877 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4855 matched stars entering correct_measured_positions(), 14576 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 4855 matched stars entering correct_measured_positions(), 14576 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 4855 stars left (next iteration limit 5340)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits N_match=4855 sigma_overall_arcsec=0.504 sigma_q1_arcsec=0.641 sigma_q2_arcsec=0.562 sigma_q3_arcsec=0.453 sigma_q4_arcsec=0.446 n_q1=1023 n_q2=1167 n_q3=1286 n_q4=1379 worst_quadrant_to_overall_ratio=1.270
The image catalog is written to wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-09-Q1b1x1_023236_TTUQ1b1x1_3652972_3vDyaYLu/fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits -region wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.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_2026-08-06_CI_Cam-09-Q1b1x1_023236_TTUQ1b1x1_3652972_3vDyaYLu/wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-30-03_20.00sec_-0.00C_LIGHTs_0276.fits
Saving fully-calibrated image wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.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_2026-08-06_CI_Cam-09-Q1b1x1_023236_TTUQ1b1x1_3652972_3vDyaYLu/wcs_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277.fits
Preparing the HTML report for the field Cam-09-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:33:22.20 +61:37:46.7: 11.89 +/- 0.01 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:38:55.63 +61:27:37.6: 11.56 +/- 0.01 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:25:02.32 +59:26:05.8: 11.99 +/- 0.01 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 04:02:14.34 +62:43:48.3: 12.34 +/- 0.01 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:13:10.70 +57:30:22.5: 12.39 +/- 0.01 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:33:22.20 +61:37:46.7: 11.89 +/- 0.01 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:38:55.63 +61:27:37.6: 11.55 +/- 0.01 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:25:41.62 +59:44:54.0: 12.40 +/- 0.01 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 04:25:53.05 +64:32:55.6: 12.53 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.89 +/- 0.00
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:25:02.32 +59:26:05.8: 11.99 +/- 0.01 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 04:02:17.59 +62:46:21.5: 12.45 +/- 0.01 detection
Forced photometry filter KEPT candidate at 05:33:22.20 +61:37:46.7: ref_mag=11.89 +/- 0.00 new_mean_mag=10.8084 delta=1.08 (need > 0.90)
Forced photometry reference-image weighted average: 11.55 +/- 0.00
Forced photometry filter KEPT candidate at 05:38:55.63 +61:27:37.6: ref_mag=11.55 +/- 0.00 new_mean_mag=10.4880 delta=1.06 (need > 0.90)
Forced photometry reference-image weighted average: 11.99 +/- 0.01
Forced photometry filter KEPT candidate at 05:25:02.32 +59:26:05.8: ref_mag=11.99 +/- 0.01 new_mean_mag=10.7333 delta=1.26 (need > 0.90)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:13:10.70 +57:30:22.5: 12.35 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.37 +/- 0.01
Forced photometry filter KEPT candidate at 05:13:10.70 +57:30:22.5: ref_mag=12.37 +/- 0.01 new_mean_mag=11.4567 delta=0.91 (need > 0.90)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 04:02:14.34 +62:43:48.3: 12.30 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.32 +/- 0.01
Forced photometry filter KEPT candidate at 04:02:14.34 +62:43:48.3: ref_mag=12.32 +/- 0.01 new_mean_mag=11.3427 delta=0.98 (need > 0.90)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:32:23.46 +60:58:24.7: 12.55 +/- 0.01 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 04:03:00.53 +63:28:10.4: 12.60 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 04:25:53.05 +64:32:55.6: 12.50 +/- 0.01 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:25:41.62 +59:44:54.0: 12.43 +/- 0.01 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 04:02:17.59 +62:46:21.5: 12.46 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.42 +/- 0.01
Forced photometry reference-image weighted average: 12.52 +/- 0.01
Forced photometry filter KEPT candidate at 05:25:41.62 +59:44:54.0: ref_mag=12.42 +/- 0.01 new_mean_mag=11.2849 delta=1.13 (need > 0.90)
Forced photometry filter KEPT candidate at 04:25:53.05 +64:32:55.6: ref_mag=12.52 +/- 0.01 new_mean_mag=11.5378 delta=0.98 (need > 0.90)
Forced photometry reference-image weighted average: 12.46 +/- 0.01
Forced photometry filter KEPT candidate at 04:02:17.59 +62:46:21.5: ref_mag=12.46 +/- 0.01 new_mean_mag=11.5165 delta=0.94 (need > 0.90)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 04:03:00.53 +63:28:10.4: 12.59 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:32:23.46 +60:58:24.7: 12.56 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.55 +/- 0.01
Forced photometry reference-image weighted average: 12.59 +/- 0.01
Forced photometry filter KEPT candidate at 05:32:23.46 +60:58:24.7: ref_mag=12.55 +/- 0.01 new_mean_mag=11.5757 delta=0.98 (need > 0.90)
Forced photometry filter KEPT candidate at 04:03:00.53 +63:28:10.4: ref_mag=12.59 +/- 0.01 new_mean_mag=11.6296 delta=0.96 (need > 0.90)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:12:10.10 +57:29:30.2: 12.61 +/- 0.01 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:31:45.06 +60:52:54.3: 12.61 +/- 0.01 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:17:23.98 +59:04:48.3: 12.64 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:12:10.10 +57:29:30.2: 12.60 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.01
Forced photometry filter KEPT candidate at 05:12:10.10 +57:29:30.2: ref_mag=12.61 +/- 0.01 new_mean_mag=11.4624 delta=1.14 (need > 0.90)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:31:45.06 +60:52:54.3: 12.60 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.01
Forced photometry filter KEPT candidate at 05:31:45.06 +60:52:54.3: ref_mag=12.61 +/- 0.01 new_mean_mag=11.6053 delta=1.00 (need > 0.90)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 03:59:56.49 +64:34:11.7: 12.67 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:17:23.98 +59:04:48.3: 12.61 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.01
Forced photometry filter KEPT candidate at 05:17:23.98 +59:04:48.3: ref_mag=12.63 +/- 0.01 new_mean_mag=11.6038 delta=1.02 (need > 0.90)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:34:18.58 +61:23:55.3: 12.78 +/- 0.01 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 03:59:56.49 +64:34:11.7: 12.73 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.69 +/- 0.01
Forced photometry filter KEPT candidate at 03:59:56.49 +64:34:11.7: ref_mag=12.69 +/- 0.01 new_mean_mag=11.6800 delta=1.01 (need > 0.90)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:34:18.58 +61:23:55.3: 12.77 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.01
Forced photometry filter KEPT candidate at 05:34:18.58 +61:23:55.3: ref_mag=12.77 +/- 0.01 new_mean_mag=11.8443 delta=0.93 (need > 0.90)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:16:44.15 +58:21:23.9: 12.84 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:31:58.29 +60:29:28.1: 12.79 +/- 0.01 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:16:44.15 +58:21:23.9: 12.87 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:31:58.29 +60:29:28.1: 12.81 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.01
Forced photometry filter KEPT candidate at 05:16:44.15 +58:21:23.9: ref_mag=12.85 +/- 0.01 new_mean_mag=11.5276 delta=1.32 (need > 0.90)
Forced photometry reference-image weighted average: 12.80 +/- 0.01
Forced photometry filter KEPT candidate at 05:31:58.29 +60:29:28.1: ref_mag=12.80 +/- 0.01 new_mean_mag=11.8429 delta=0.96 (need > 0.90)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:27:18.39 +57:34:43.0: 12.89 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:27:18.39 +57:34:43.0: 12.86 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.87 +/- 0.01
Forced photometry filter KEPT candidate at 05:27:18.39 +57:34:43.0: ref_mag=12.87 +/- 0.01 new_mean_mag=11.8495 delta=1.02 (need > 0.90)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:20:45.19 +59:10:52.5: 12.93 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:20:41.53 +58:47:16.6: 12.90 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:24:42.31 +60:06:59.4: 12.91 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:24:24.61 +62:37:45.6: 12.98 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:20:45.19 +59:10:52.5: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.01
Forced photometry filter KEPT candidate at 05:20:45.19 +59:10:52.5: ref_mag=12.92 +/- 0.01 new_mean_mag=11.8944 delta=1.03 (need > 0.90)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:20:41.53 +58:47:16.6: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.01
Forced photometry filter KEPT candidate at 05:20:41.53 +58:47:16.6: ref_mag=12.90 +/- 0.01 new_mean_mag=11.6121 delta=1.29 (need > 0.90)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:24:42.31 +60:06:59.4: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.01
Forced photometry filter KEPT candidate at 05:24:42.31 +60:06:59.4: ref_mag=12.91 +/- 0.01 new_mean_mag=11.9358 delta=0.98 (need > 0.90)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:24:24.61 +62:37:45.6: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.01
Forced photometry filter KEPT candidate at 05:24:24.61 +62:37:45.6: ref_mag=12.95 +/- 0.01 new_mean_mag=11.8530 delta=1.09 (need > 0.90)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:33:37.69 +63:19:21.7: 13.11 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:36:55.58 +60:53:52.4: 13.51 +/- 0.03 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:33:37.69 +63:19:21.7: 13.17 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Forced photometry filter KEPT candidate at 05:33:37.69 +63:19:21.7: ref_mag=13.14 +/- 0.02 new_mean_mag=11.9455 delta=1.19 (need > 0.90)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:48:40.56 +62:22:30.8: 12.98 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:36:55.58 +60:53:52.4: 13.54 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.53 +/- 0.02
Forced photometry filter KEPT candidate at 05:36:55.58 +60:53:52.4: ref_mag=13.53 +/- 0.02 new_mean_mag=12.3152 delta=1.21 (need > 0.90)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:48:40.56 +62:22:30.8: 12.89 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.01
Forced photometry filter REJECTED candidate at 05:48:40.56 +62:22:30.8: ref_mag=12.94 +/- 0.01 new_mean_mag=12.1476 delta=0.79 (need > 0.90)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:15:23.63 +58:19:51.5: 13.26 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:30:55.18 +60:37:14.4: 13.25 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:15:23.63 +58:19:51.5: 13.24 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.25 +/- 0.02
Forced photometry filter KEPT candidate at 05:15:23.63 +58:19:51.5: ref_mag=13.25 +/- 0.02 new_mean_mag=12.1004 delta=1.15 (need > 0.90)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:30:55.18 +60:37:14.4: 13.30 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.02
Forced photometry filter KEPT candidate at 05:30:55.18 +60:37:14.4: ref_mag=13.28 +/- 0.02 new_mean_mag=12.1105 delta=1.16 (need > 0.90)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:16:10.93 +57:59:19.4: 13.25 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:16:10.93 +57:59:19.4: 13.30 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.02
Forced photometry filter KEPT candidate at 05:16:10.93 +57:59:19.4: ref_mag=13.27 +/- 0.02 new_mean_mag=11.9666 delta=1.31 (need > 0.90)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:31:48.36 +60:08:44.4: 13.10 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:41:43.20 +63:49:54.5: 13.11 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:31:48.36 +60:08:44.4: 13.12 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.01
Forced photometry filter KEPT candidate at 05:31:48.36 +60:08:44.4: ref_mag=13.11 +/- 0.01 new_mean_mag=12.0745 delta=1.04 (need > 0.90)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:41:43.20 +63:49:54.5: 13.09 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.01
Forced photometry filter KEPT candidate at 05:41:43.20 +63:49:54.5: ref_mag=13.10 +/- 0.01 new_mean_mag=12.1019 delta=1.00 (need > 0.90)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:30:04.50 +59:48:06.6: 13.09 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:30:04.50 +59:48:06.6: 13.11 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.01
Forced photometry filter KEPT candidate at 05:30:04.50 +59:48:06.6: ref_mag=13.10 +/- 0.01 new_mean_mag=12.0427 delta=1.05 (need > 0.90)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:24:37.77 +57:14:43.8: 12.98 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:24:37.77 +57:14:43.8: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.01
Forced photometry filter KEPT candidate at 05:24:37.77 +57:14:43.8: ref_mag=12.96 +/- 0.01 new_mean_mag=11.8852 delta=1.08 (need > 0.90)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:17:31.83 +57:49:59.7: 12.99 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:17:31.83 +57:49:59.7: 12.96 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.01
Forced photometry filter KEPT candidate at 05:17:31.83 +57:49:59.7: ref_mag=12.98 +/- 0.01 new_mean_mag=11.8550 delta=1.12 (need > 0.90)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:29:10.96 +60:36:41.9: 12.96 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:29:10.96 +60:36:41.9: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.01
Forced photometry filter KEPT candidate at 05:29:10.96 +60:36:41.9: ref_mag=12.94 +/- 0.01 new_mean_mag=11.8888 delta=1.05 (need > 0.90)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 04:01:03.27 +63:13:15.3: 12.93 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 04:01:03.27 +63:13:15.3: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.02
Forced photometry filter KEPT candidate at 04:01:03.27 +63:13:15.3: ref_mag=12.91 +/- 0.02 new_mean_mag=11.7570 delta=1.15 (need > 0.90)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:17:24.51 +57:39:29.5: 12.93 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:17:24.51 +57:39:29.5: 12.91 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.01
Forced photometry filter KEPT candidate at 05:17:24.51 +57:39:29.5: ref_mag=12.92 +/- 0.01 new_mean_mag=11.9222 delta=1.00 (need > 0.90)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:30:17.92 +60:13:29.3: 12.94 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:30:17.92 +60:13:29.3: 12.95 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.01
Forced photometry filter KEPT candidate at 05:30:17.92 +60:13:29.3: ref_mag=12.95 +/- 0.01 new_mean_mag=11.9519 delta=1.00 (need > 0.90)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:20:23.60 +58:15:45.7: 12.93 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:20:23.60 +58:15:45.7: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.01
Forced photometry filter KEPT candidate at 05:20:23.60 +58:15:45.7: ref_mag=12.91 +/- 0.01 new_mean_mag=11.8905 delta=1.02 (need > 0.90)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:33:25.57 +59:36:24.0: 12.90 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:33:25.57 +59:36:24.0: 12.95 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.01
Forced photometry filter KEPT candidate at 05:33:25.57 +59:36:24.0: ref_mag=12.92 +/- 0.01 new_mean_mag=11.7364 delta=1.19 (need > 0.90)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:47:24.44 +62:54:04.0: 12.88 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:47:24.44 +62:54:04.0: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.01
Forced photometry filter KEPT candidate at 05:47:24.44 +62:54:04.0: ref_mag=12.89 +/- 0.01 new_mean_mag=11.9258 delta=0.97 (need > 0.90)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:11:31.50 +60:06:25.0: 12.87 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:12:16.18 +57:24:20.6: 12.87 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:11:31.50 +60:06:25.0: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.01
Forced photometry filter KEPT candidate at 05:11:31.50 +60:06:25.0: ref_mag=12.89 +/- 0.01 new_mean_mag=11.9045 delta=0.98 (need > 0.90)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:12:16.18 +57:24:20.6: 12.85 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.01
Forced photometry filter KEPT candidate at 05:12:16.18 +57:24:20.6: ref_mag=12.86 +/- 0.01 new_mean_mag=11.8829 delta=0.97 (need > 0.90)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:25:54.62 +59:36:04.4: 12.84 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:25:54.62 +59:36:04.4: 12.79 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.01
Forced photometry filter KEPT candidate at 05:25:54.62 +59:36:04.4: ref_mag=12.81 +/- 0.01 new_mean_mag=11.7358 delta=1.08 (need > 0.90)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:19:19.08 +58:49:11.1: 12.80 +/- 0.01 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:19:19.08 +58:49:11.1: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.01
Forced photometry filter KEPT candidate at 05:19:19.08 +58:49:11.1: ref_mag=12.81 +/- 0.01 new_mean_mag=11.6559 delta=1.15 (need > 0.90)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:11:25.37 +57:58:22.1: 12.76 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:32:22.89 +60:40:32.8: 12.75 +/- 0.01 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:11:25.37 +57:58:22.1: 12.78 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.01
Forced photometry filter KEPT candidate at 05:11:25.37 +57:58:22.1: ref_mag=12.77 +/- 0.01 new_mean_mag=11.7298 delta=1.04 (need > 0.90)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 04:06:25.67 +62:15:49.9: 12.76 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:32:22.89 +60:40:32.8: 12.80 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.01
Forced photometry filter KEPT candidate at 05:32:22.89 +60:40:32.8: ref_mag=12.78 +/- 0.01 new_mean_mag=11.7955 delta=0.98 (need > 0.90)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 04:06:25.67 +62:15:49.9: 12.74 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.75 +/- 0.01
Forced photometry filter KEPT candidate at 04:06:25.67 +62:15:49.9: ref_mag=12.75 +/- 0.01 new_mean_mag=11.7191 delta=1.03 (need > 0.90)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:31:48.63 +59:43:20.3: 12.79 +/- 0.01 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:31:48.63 +59:43:20.3: 12.78 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.01
Forced photometry filter KEPT candidate at 05:31:48.63 +59:43:20.3: ref_mag=12.78 +/- 0.01 new_mean_mag=11.8389 delta=0.95 (need > 0.90)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:32:25.55 +60:40:50.5: 12.73 +/- 0.01 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:32:25.55 +60:40:50.5: 12.72 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.73 +/- 0.01
Forced photometry filter KEPT candidate at 05:32:25.55 +60:40:50.5: ref_mag=12.73 +/- 0.01 new_mean_mag=11.7357 delta=0.99 (need > 0.90)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:26:21.42 +60:17:36.9: 12.73 +/- 0.01 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:29:58.65 +61:00:42.8: 12.70 +/- 0.01 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:26:21.42 +60:17:36.9: 12.72 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.72 +/- 0.01
Forced photometry filter KEPT candidate at 05:26:21.42 +60:17:36.9: ref_mag=12.72 +/- 0.01 new_mean_mag=11.7499 delta=0.98 (need > 0.90)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:36:07.53 +60:03:31.3: 12.66 +/- 0.01 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:29:58.65 +61:00:42.8: 12.67 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.01
Forced photometry filter KEPT candidate at 05:29:58.65 +61:00:42.8: ref_mag=12.68 +/- 0.01 new_mean_mag=11.5239 delta=1.16 (need > 0.90)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 04:22:13.42 +62:59:34.8: 12.62 +/- 0.01 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:36:07.53 +60:03:31.3: 12.64 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.01
Forced photometry filter KEPT candidate at 05:36:07.53 +60:03:31.3: ref_mag=12.65 +/- 0.01 new_mean_mag=11.7283 delta=0.92 (need > 0.90)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 04:22:13.42 +62:59:34.8: 12.65 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.01
Forced photometry filter KEPT candidate at 04:22:13.42 +62:59:34.8: ref_mag=12.63 +/- 0.01 new_mean_mag=11.6549 delta=0.98 (need > 0.90)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 04:04:20.63 +63:26:50.0: 12.61 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 04:04:20.63 +63:26:50.0: 12.57 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.59 +/- 0.01
Forced photometry filter KEPT candidate at 04:04:20.63 +63:26:50.0: ref_mag=12.59 +/- 0.01 new_mean_mag=11.6369 delta=0.95 (need > 0.90)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 04:00:49.34 +64:12:08.8: 12.53 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 04:02:52.89 +62:32:54.0: 12.50 +/- 0.02 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 04:00:49.34 +64:12:08.8: 12.58 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.56 +/- 0.01
Forced photometry filter KEPT candidate at 04:00:49.34 +64:12:08.8: ref_mag=12.56 +/- 0.01 new_mean_mag=11.6187 delta=0.94 (need > 0.90)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 04:02:52.89 +62:32:54.0: 12.49 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.49 +/- 0.01
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:25:16.39 +58:59:13.0: 12.50 +/- 0.01 detection
Forced photometry filter KEPT candidate at 04:02:52.89 +62:32:54.0: ref_mag=12.49 +/- 0.01 new_mean_mag=11.4621 delta=1.03 (need > 0.90)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:25:16.39 +58:59:13.0: 12.54 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.52 +/- 0.01
Forced photometry filter KEPT candidate at 05:25:16.39 +58:59:13.0: ref_mag=12.52 +/- 0.01 new_mean_mag=11.5242 delta=1.00 (need > 0.90)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:36:29.67 +60:26:04.3: 12.49 +/- 0.01 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:36:29.67 +60:26:04.3: 12.52 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.50 +/- 0.01
Forced photometry filter KEPT candidate at 05:36:29.67 +60:26:04.3: ref_mag=12.50 +/- 0.01 new_mean_mag=11.5144 delta=0.99 (need > 0.90)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:18:55.15 +58:43:40.0: 12.48 +/- 0.01 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:18:55.15 +58:43:40.0: 12.46 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.47 +/- 0.01
Forced photometry filter KEPT candidate at 05:18:55.15 +58:43:40.0: ref_mag=12.47 +/- 0.01 new_mean_mag=11.4018 delta=1.07 (need > 0.90)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:28:38.93 +57:14:48.0: 12.40 +/- 0.01 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:28:38.93 +57:14:48.0: 12.40 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.40 +/- 0.01
Forced photometry filter KEPT candidate at 05:28:38.93 +57:14:48.0: ref_mag=12.40 +/- 0.01 new_mean_mag=11.4543 delta=0.95 (need > 0.90)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:27:56.83 +61:23:37.2: 12.35 +/- 0.01 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:27:56.83 +61:23:37.2: 12.37 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.36 +/- 0.01
Forced photometry filter KEPT candidate at 05:27:56.83 +61:23:37.2: ref_mag=12.36 +/- 0.01 new_mean_mag=11.2427 delta=1.12 (need > 0.90)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 04:13:24.14 +60:25:32.9: 12.30 +/- 0.01 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 04:13:24.14 +60:25:32.9: 12.33 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.32 +/- 0.01
Forced photometry filter KEPT candidate at 04:13:24.14 +60:25:32.9: ref_mag=12.32 +/- 0.01 new_mean_mag=11.4131 delta=0.90 (need > 0.90)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 04:03:08.77 +62:16:12.3: 12.26 +/- 0.01 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 04:03:08.77 +62:16:12.3: 12.26 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.26 +/- 0.01
Forced photometry filter KEPT candidate at 04:03:08.77 +62:16:12.3: ref_mag=12.26 +/- 0.01 new_mean_mag=11.2702 delta=0.99 (need > 0.90)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:52:46.58 +62:41:17.9: 12.17 +/- 0.01 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:52:46.58 +62:41:17.9: 12.18 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.18 +/- 0.01
Forced photometry filter KEPT candidate at 05:52:46.58 +62:41:17.9: ref_mag=12.18 +/- 0.01 new_mean_mag=11.1285 delta=1.05 (need > 0.90)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:24:12.11 +57:31:54.1: 12.01 +/- 0.01 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:24:12.11 +57:31:54.1: 11.99 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.00 +/- 0.01
Forced photometry filter KEPT candidate at 05:24:12.11 +57:31:54.1: ref_mag=12.00 +/- 0.01 new_mean_mag=11.0299 delta=0.97 (need > 0.90)
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits at 05:10:13.79 +57:18:18.8: 11.99 +/- 0.01 detection
Forced photometry on wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits at 05:10:13.79 +57:18:18.8: 12.01 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.00 +/- 0.01
Forced photometry filter KEPT candidate at 05:10:13.79 +57:18:18.8: ref_mag=12.00 +/- 0.01 new_mean_mag=11.0533 delta=0.94 (need > 0.90)
Adding exclusion_list_local.txt__out03680.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04233.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07026.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07708.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08066.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08215.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09020.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09021.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10408.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out105438.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out108072.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out109058.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out109814.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116289.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116821.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out119348.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out122571.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out123661.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out124663.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12732.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out129190.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14895.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15362.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17907.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19507.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19692.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24125.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24772.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25120.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26843.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out28971.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29951.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32295.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34152.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34564.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35654.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36398.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36896.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39831.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41199.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41463.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out42360.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out43007.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out43584.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44653.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out45877.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out47503.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out47618.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out48207.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out48261.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50858.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51037.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52058.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52755.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out57264.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out57703.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out57738.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out60390.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out68254.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out74288.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out74532.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77982.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out91238.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out92596.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out98134.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 64s
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: 32s
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Considering the candidate 152542_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
The candidate 152542_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277 did not pass the final checks
**** FOUND 04:40:16.97 +66:08:06.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 152897_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
The candidate 152897_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277 did not pass the final checks
**** FOUND 05:57:46.48 +66:05:16.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 152925_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
The candidate 152925_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277 did not pass the final checks
**** FOUND 05:06:21.14 +58:57:52.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 153106_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
The candidate 153106_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277 did not pass the final checks
**** FOUND 04:39:32.46 +63:12:32.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 46344_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
The candidate 46344_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277 did not pass the final checks
**** FOUND 05:03:25.26 +60:26:31.8 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 101295_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
The candidate 101295_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277 did not pass the final checks
**** FOUND 04:38:05.68 +65:13:57.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57264_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 57264_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
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Considering the candidate 111330_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
The candidate 111330_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277 did not pass the final checks
**** FOUND 05:30:42.38 +65:12:40.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 60390_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 60390_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
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Considering the candidate 32295_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 32295_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
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Considering the candidate 28320_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
The candidate 28320_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277 did not pass the final checks
**** FOUND 05:29:44.69 +59:09:27.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 116821_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 116821_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
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Considering the candidate 43092_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
The candidate 43092_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277 did not pass the final checks
**** FOUND 05:14:53.83 +60:10:30.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 09020_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 09020_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
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Considering the candidate 36398_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 36398_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
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Considering the candidate 116289_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 116289_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
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Considering the candidate 105438_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 105438_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
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Considering the candidate 52058_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 52058_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
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Considering the candidate 108072_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 108072_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
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Considering the candidate 09021_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 09021_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
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Considering the candidate 50858_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 50858_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
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Considering the candidate 28971_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 28971_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
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Considering the candidate 91238_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 91238_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
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Considering the candidate 57703_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 57703_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
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Considering the candidate 45877_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 45877_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
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Considering the candidate 19507_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 19507_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
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Considering the candidate 08215_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 08215_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
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Considering the candidate 29951_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 29951_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
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Considering the candidate 24772_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 24772_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
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Considering the candidate 41463_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 41463_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
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Considering the candidate 74532_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 74532_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
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Considering the candidate 92596_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 92596_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
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Considering the candidate 121037_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
The candidate 121037_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277 did not pass the final checks
**** FOUND 05:19:46.07 +64:26:02.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 51037_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 51037_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
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Considering the candidate 61169_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
The candidate 61169_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277 did not pass the final checks
Rejecting candidate due to large distance (46.5") between the two second-epoch detections
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Considering the candidate 71006_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
The candidate 71006_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277 did not pass the final checks
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Considering the candidate 123760_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
The candidate 123760_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277 did not pass the final checks
**** FOUND 05:47:14.21 +64:15:50.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 43617_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
The candidate 43617_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277 did not pass the final checks
**** FOUND 04:14:55.83 +58:31:15.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 19692_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 19692_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
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Considering the candidate 47618_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 47618_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
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Considering the candidate 10998_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
The candidate 10998_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277 did not pass the final checks
**** FOUND 05:28:18.79 +57:48:46.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 14895_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 14895_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
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Considering the candidate 124436_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
The candidate 124436_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277 did not pass the final checks
**** FOUND 05:14:38.43 +64:06:22.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 11549_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
The candidate 11549_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277 did not pass the final checks
**** FOUND 05:33:59.25 +57:53:38.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 41199_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 41199_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
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Considering the candidate 129190_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 129190_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
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Considering the candidate 36896_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 36896_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
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Considering the candidate 124794_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
The candidate 124794_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277 did not pass the final checks
**** FOUND 05:48:25.90 +64:11:32.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 04233_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 04233_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
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Considering the candidate 12732_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 12732_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
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Considering the candidate 81854_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
The candidate 81854_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277 did not pass the final checks
**** FOUND 04:35:17.66 +62:16:24.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 47503_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 47503_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
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Considering the candidate 109814_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 109814_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
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Considering the candidate 10408_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 10408_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
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Considering the candidate 48062_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
The candidate 48062_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277 did not pass the final checks
**** FOUND 05:25:45.76 +60:38:43.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 42360_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 42360_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
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Considering the candidate 17907_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 17907_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
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Considering the candidate 34152_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 34152_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
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Considering the candidate 77982_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 77982_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
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Considering the candidate 43007_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 43007_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
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Considering the candidate 08066_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 08066_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
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Considering the candidate 34564_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 34564_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
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Considering the candidate 127704_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
The candidate 127704_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277 did not pass the final checks
**** FOUND 05:48:02.11 +63:56:31.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 71135_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
The candidate 71135_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277 did not pass the final checks
**** FOUND 05:10:46.09 +62:14:02.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 25120_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 25120_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
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Considering the candidate 15362_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 15362_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
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Considering the candidate 48261_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 48261_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
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Considering the candidate 124663_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 124663_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
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Considering the candidate 35654_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 35654_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
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Considering the candidate 48207_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 48207_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
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Considering the candidate 43584_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 43584_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
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Considering the candidate 52755_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 52755_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
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Considering the candidate 39831_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 39831_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
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Considering the candidate 123661_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 123661_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
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Considering the candidate 109058_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 109058_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
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Considering the candidate 43781_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
The candidate 43781_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277 did not pass the final checks
**** FOUND 04:14:09.79 +58:31:29.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 98134_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 98134_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
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Considering the candidate 119348_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 119348_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
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Considering the candidate 26843_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 26843_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
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Considering the candidate 44653_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 44653_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
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Considering the candidate 24125_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 24125_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
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Considering the candidate 03680_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 03680_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
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Considering the candidate 57738_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 57738_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68254_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 68254_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 122571_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 122571_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74288_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 74288_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29771_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
The candidate 29771_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277 did not pass the final checks
**** FOUND 04:19:08.66 +57:38:25.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07708_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 07708_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07026_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 07026_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 114136_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
The candidate 114136_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277 did not pass the final checks
**** FOUND 05:58:38.93 +63:43:51.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 78569_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
The candidate 78569_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277 did not pass the final checks
**** FOUND 05:53:45.16 +63:00:50.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72637_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
The candidate 72637_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277 did not pass the final checks
**** FOUND 05:20:22.44 +62:39:10.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 126795_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
The candidate 126795_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277 did not pass the final checks
**** FOUND 04:52:05.57 +63:30:14.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32056_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
The candidate 32056_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277 did not pass the final checks
**** FOUND 05:15:11.50 +59:24:20.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 78190_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
The candidate 78190_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277 did not pass the final checks
**** FOUND 05:30:09.94 +63:03:59.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 28091_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
The candidate 28091_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277 did not pass the final checks
**** FOUND 05:06:08.49 +58:58:22.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 89933_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
The candidate 89933_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277 did not pass the final checks
**** FOUND 04:54:03.26 +66:20:30.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05929_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
The candidate 05929_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277 did not pass the final checks
**** FOUND 05:23:27.75 +57:32:39.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 65521_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277
The candidate 65521_fd_Cam-09-Q1b1x1_2026-08-06_02-31-00_20.00sec_-0.00C_LIGHTs_0277 did not pass the final checks
**** FOUND 04:21:48.15 +60:44:05.0 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 4s
make_report_in_HTML.sh TOTAL: 100s
Prepared the HTML report for the field Cam-09-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
05:28:38.93 +57:14:48.0
05:24:37.77 +57:14:43.8
05:10:13.79 +57:18:18.8
05:24:12.11 +57:31:54.1
05:12:16.18 +57:24:20.6
05:27:18.39 +57:34:43.0
05:13:10.70 +57:30:22.5
05:12:10.10 +57:29:30.2
05:17:24.51 +57:39:29.5
04:25:53.05 +64:32:55.6
04:03:00.53 +63:28:10.4
04:04:20.63 +63:26:50.0
04:01:03.27 +63:13:15.3
04:02:17.59 +62:46:21.5
04:02:14.34 +62:43:48.3
04:02:52.89 +62:32:54.0
04:03:08.77 +62:16:12.3
04:22:13.42 +62:59:34.8
04:06:25.67 +62:15:49.9
05:17:31.83 +57:49:59.7
05:41:43.20 +63:49:54.5
05:16:10.93 +57:59:19.4
05:11:25.37 +57:58:22.1
05:20:23.60 +58:15:45.7
05:16:44.15 +58:21:23.9
05:15:23.63 +58:19:51.5
05:18:55.15 +58:43:40.0
05:20:41.53 +58:47:16.6
05:19:19.08 +58:49:11.1
05:25:16.39 +58:59:13.0
05:17:23.98 +59:04:48.3
05:20:45.19 +59:10:52.5
05:25:02.32 +59:26:05.8
05:33:25.57 +59:36:24.0
05:25:54.62 +59:36:04.4
05:31:48.63 +59:43:20.3
05:25:41.62 +59:44:54.0
05:30:04.50 +59:48:06.6
05:36:07.53 +60:03:31.3
05:31:48.36 +60:08:44.4
05:24:42.31 +60:06:59.4
05:30:17.92 +60:13:29.3
05:11:31.50 +60:06:25.0
05:26:21.42 +60:17:36.9
05:36:29.67 +60:26:04.3
05:31:58.29 +60:29:28.1
05:29:10.96 +60:36:41.9
05:30:55.18 +60:37:14.4
05:32:25.55 +60:40:50.5
05:32:22.89 +60:40:32.8
05:31:45.06 +60:52:54.3
05:36:55.58 +60:53:52.4
05:32:23.46 +60:58:24.7
05:29:58.65 +61:00:42.8
05:38:55.63 +61:27:37.6
05:34:18.58 +61:23:55.3
05:27:56.83 +61:23:37.2
05:33:22.20 +61:37:46.7
04:13:24.14 +60:25:32.9
05:52:46.58 +62:41:17.9
05:24:24.61 +62:37:45.6
05:47:24.44 +62:54:04.0
03:59:56.49 +64:34:11.7
05:33:37.69 +63:19:21.7
04:00:49.34 +64:12:08.8
########### Completed Cam-09-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
05:38:55.63 +61:27:37.6
05:33:22.20 +61:37:46.7
05:25:02.32 +59:26:05.8
04:02:14.34 +62:43:48.3
05:13:10.70 +57:30:22.5
05:25:41.62 +59:44:54.0
04:02:17.59 +62:46:21.5
04:25:53.05 +64:32:55.6
05:32:23.46 +60:58:24.7
04:03:00.53 +63:28:10.4
05:12:10.10 +57:29:30.2
05:31:45.06 +60:52:54.3
05:17:23.98 +59:04:48.3
03:59:56.49 +64:34:11.7
05:34:18.58 +61:23:55.3
05:31:58.29 +60:29:28.1
05:16:44.15 +58:21:23.9
05:27:18.39 +57:34:43.0
05:20:45.19 +59:10:52.5
05:20:41.53 +58:47:16.6
05:24:42.31 +60:06:59.4
05:24:24.61 +62:37:45.6
05:33:37.69 +63:19:21.7
05:36:55.58 +60:53:52.4
05:15:23.63 +58:19:51.5
05:30:55.18 +60:37:14.4
05:16:10.93 +57:59:19.4
05:31:48.36 +60:08:44.4
05:41:43.20 +63:49:54.5
05:30:04.50 +59:48:06.6
05:24:37.77 +57:14:43.8
05:17:31.83 +57:49:59.7
05:29:10.96 +60:36:41.9
04:01:03.27 +63:13:15.3
05:17:24.51 +57:39:29.5
05:30:17.92 +60:13:29.3
05:20:23.60 +58:15:45.7
05:33:25.57 +59:36:24.0
05:47:24.44 +62:54:04.0
05:11:31.50 +60:06:25.0
05:12:16.18 +57:24:20.6
05:25:54.62 +59:36:04.4
05:19:19.08 +58:49:11.1
05:11:25.37 +57:58:22.1
05:32:22.89 +60:40:32.8
04:06:25.67 +62:15:49.9
05:31:48.63 +59:43:20.3
05:32:25.55 +60:40:50.5
05:26:21.42 +60:17:36.9
05:29:58.65 +61:00:42.8
05:36:07.53 +60:03:31.3
04:22:13.42 +62:59:34.8
04:04:20.63 +63:26:50.0
04:00:49.34 +64:12:08.8
04:02:52.89 +62:32:54.0
05:25:16.39 +58:59:13.0
05:36:29.67 +60:26:04.3
05:18:55.15 +58:43:40.0
05:28:38.93 +57:14:48.0
05:27:56.83 +61:23:37.2
04:13:24.14 +60:25:32.9
04:03:08.77 +62:16:12.3
05:52:46.58 +62:41:17.9
05:24:12.11 +57:31:54.1
05:10:13.79 +57:18:18.8
###################################################################################
05:38:55.63 +61:27:37.6 -- not an asteroid (will add it to exclusion list)
05:33:22.20 +61:37:46.7 -- not an asteroid (will add it to exclusion list)
05:25:02.32 +59:26:05.8 -- not an asteroid (will add it to exclusion list)
04:02:14.34 +62:43:48.3 -- not an asteroid (will add it to exclusion list)
05:13:10.70 +57:30:22.5 -- not an asteroid (will add it to exclusion list)
05:25:41.62 +59:44:54.0 -- not an asteroid (will add it to exclusion list)
04:02:17.59 +62:46:21.5 -- not an asteroid (will add it to exclusion list)
04:25:53.05 +64:32:55.6 -- not an asteroid (will add it to exclusion list)
05:32:23.46 +60:58:24.7 -- not an asteroid (will add it to exclusion list)
04:03:00.53 +63:28:10.4 -- not an asteroid (will add it to exclusion list)
05:12:10.10 +57:29:30.2 -- not an asteroid (will add it to exclusion list)
05:31:45.06 +60:52:54.3 -- not an asteroid (will add it to exclusion list)
05:17:23.98 +59:04:48.3 -- not an asteroid (will add it to exclusion list)
03:59:56.49 +64:34:11.7 -- not an asteroid (will add it to exclusion list)
05:34:18.58 +61:23:55.3 -- not an asteroid (will add it to exclusion list)
05:31:58.29 +60:29:28.1 -- not an asteroid (will add it to exclusion list)
05:16:44.15 +58:21:23.9 -- not an asteroid (will add it to exclusion list)
05:27:18.39 +57:34:43.0 -- not an asteroid (will add it to exclusion list)
05:20:45.19 +59:10:52.5 -- not an asteroid (will add it to exclusion list)
05:20:41.53 +58:47:16.6 -- not an asteroid (will add it to exclusion list)
05:24:42.31 +60:06:59.4 -- not an asteroid (will add it to exclusion list)
05:24:24.61 +62:37:45.6 -- not an asteroid (will add it to exclusion list)
05:33:37.69 +63:19:21.7 -- not an asteroid (will add it to exclusion list)
05:36:55.58 +60:53:52.4 -- not an asteroid (will add it to exclusion list)
05:15:23.63 +58:19:51.5 -- not an asteroid (will add it to exclusion list)
05:30:55.18 +60:37:14.4 -- not an asteroid (will add it to exclusion list)
05:16:10.93 +57:59:19.4 -- not an asteroid (will add it to exclusion list)
05:31:48.36 +60:08:44.4 -- not an asteroid (will add it to exclusion list)
05:41:43.20 +63:49:54.5 -- not an asteroid (will add it to exclusion list)
05:30:04.50 +59:48:06.6 -- not an asteroid (will add it to exclusion list)
05:24:37.77 +57:14:43.8 -- not an asteroid (will add it to exclusion list)
05:17:31.83 +57:49:59.7 -- not an asteroid (will add it to exclusion list)
05:29:10.96 +60:36:41.9 -- not an asteroid (will add it to exclusion list)
04:01:03.27 +63:13:15.3 -- not an asteroid (will add it to exclusion list)
05:17:24.51 +57:39:29.5 -- not an asteroid (will add it to exclusion list)
05:30:17.92 +60:13:29.3 -- not an asteroid (will add it to exclusion list)
05:20:23.60 +58:15:45.7 -- not an asteroid (will add it to exclusion list)
05:33:25.57 +59:36:24.0 -- not an asteroid (will add it to exclusion list)
05:47:24.44 +62:54:04.0 -- not an asteroid (will add it to exclusion list)
05:11:31.50 +60:06:25.0 -- not an asteroid (will add it to exclusion list)
05:12:16.18 +57:24:20.6 -- not an asteroid (will add it to exclusion list)
05:25:54.62 +59:36:04.4 -- not an asteroid (will add it to exclusion list)
05:19:19.08 +58:49:11.1 -- not an asteroid (will add it to exclusion list)
05:11:25.37 +57:58:22.1 -- not an asteroid (will add it to exclusion list)
05:32:22.89 +60:40:32.8 -- not an asteroid (will add it to exclusion list)
04:06:25.67 +62:15:49.9 -- not an asteroid (will add it to exclusion list)
05:31:48.63 +59:43:20.3 -- not an asteroid (will add it to exclusion list)
05:32:25.55 +60:40:50.5 -- not an asteroid (will add it to exclusion list)
05:26:21.42 +60:17:36.9 -- not an asteroid (will add it to exclusion list)
05:29:58.65 +61:00:42.8 -- not an asteroid (will add it to exclusion list)
05:36:07.53 +60:03:31.3 -- not an asteroid (will add it to exclusion list)
04:22:13.42 +62:59:34.8 -- not an asteroid (will add it to exclusion list)
04:04:20.63 +63:26:50.0 -- not an asteroid (will add it to exclusion list)
04:00:49.34 +64:12:08.8 -- not an asteroid (will add it to exclusion list)
04:02:52.89 +62:32:54.0 -- not an asteroid (will add it to exclusion list)
05:25:16.39 +58:59:13.0 -- not an asteroid (will add it to exclusion list)
05:36:29.67 +60:26:04.3 -- not an asteroid (will add it to exclusion list)
05:18:55.15 +58:43:40.0 -- not an asteroid (will add it to exclusion list)
05:28:38.93 +57:14:48.0 -- not an asteroid (will add it to exclusion list)
05:27:56.83 +61:23:37.2 -- not an asteroid (will add it to exclusion list)
04:13:24.14 +60:25:32.9 -- not an asteroid (will add it to exclusion list)
04:03:08.77 +62:16:12.3 -- not an asteroid (will add it to exclusion list)
05:52:46.58 +62:41:17.9 -- not an asteroid (will add it to exclusion list)
05:24:12.11 +57:31:54.1 -- not an asteroid (will add it to exclusion list)
05:10:13.79 +57:18:18.8 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
03:59:56.49 +64:34:11.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:00:49.34 +64:12:08.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:01:03.27 +63:13:15.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:02:14.34 +62:43:48.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:02:17.59 +62:46:21.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:02:52.89 +62:32:54.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:03:00.53 +63:28:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:03:08.77 +62:16:12.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:04:20.63 +63:26:50.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:06:25.67 +62:15:49.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:13:24.14 +60:25:32.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:22:13.42 +62:59:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:25:53.05 +64:32:55.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:10:13.79 +57:18:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:11:25.37 +57:58:22.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:11:31.50 +60:06:25.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:12:10.10 +57:29:30.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:12:16.18 +57:24:20.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:13:10.70 +57:30:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:15:23.63 +58:19:51.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:16:10.93 +57:59:19.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:16:44.15 +58:21:23.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:23.98 +59:04:48.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:24.51 +57:39:29.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:31.83 +57:49:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:55.15 +58:43:40.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:19:19.08 +58:49:11.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:20:23.60 +58:15:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:20:41.53 +58:47:16.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:20:45.19 +59:10:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:24:12.11 +57:31:54.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:24:24.61 +62:37:45.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:24:37.77 +57:14:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:24:42.31 +60:06:59.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:25:02.32 +59:26:05.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:25:16.39 +58:59:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:25:41.62 +59:44:54.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:25:54.62 +59:36:04.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:26:21.42 +60:17:36.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:27:18.39 +57:34:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:27:56.83 +61:23:37.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:28:38.93 +57:14:48.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:29:10.96 +60:36:41.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:29:58.65 +61:00:42.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:30:04.50 +59:48:06.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:30:17.92 +60:13:29.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:30:55.18 +60:37:14.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:31:45.06 +60:52:54.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:31:48.36 +60:08:44.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:31:48.63 +59:43:20.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:31:58.29 +60:29:28.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:32:22.89 +60:40:32.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:32:23.46 +60:58:24.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:32:25.55 +60:40:50.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:33:22.20 +61:37:46.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:33:25.57 +59:36:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:33:37.69 +63:19:21.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:34:18.58 +61:23:55.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:36:07.53 +60:03:31.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:36:29.67 +60:26:04.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:36:55.58 +60:53:52.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:38:55.63 +61:27:37.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:41:43.20 +63:49:54.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:47:24.44 +62:54:04.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:46.58 +62:41:17.9 -- 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)
03:59:56.49 +64:34:11.7 -- not a known variable star
04:00:49.34 +64:12:08.8 -- not a known variable star
04:01:03.27 +63:13:15.3 -- a known variable star
04:02:14.34 +62:43:48.3 -- not a known variable star
04:02:17.59 +62:46:21.5 -- not a known variable star
04:02:52.89 +62:32:54.0 -- a known variable star
04:03:00.53 +63:28:10.4 -- not a known variable star
04:03:08.77 +62:16:12.3 -- a known variable star
04:04:20.63 +63:26:50.0 -- a known variable star
04:06:25.67 +62:15:49.9 -- a known variable star
04:13:24.14 +60:25:32.9 -- a known variable star
04:22:13.42 +62:59:34.8 -- a known variable star
04:25:53.05 +64:32:55.6 -- a known variable star
05:10:13.79 +57:18:18.8 -- not a known variable star
05:11:25.37 +57:58:22.1 -- not a known variable star
05:11:31.50 +60:06:25.0 -- not a known variable star
05:12:10.10 +57:29:30.2 -- a known variable star
05:12:16.18 +57:24:20.6 -- a known variable star
05:13:10.70 +57:30:22.5 -- not a known variable star
05:15:23.63 +58:19:51.5 -- not a known variable star
05:16:10.93 +57:59:19.4 -- not a known variable star
05:16:44.15 +58:21:23.9 -- not a known variable star
05:17:23.98 +59:04:48.3 -- not a known variable star
05:17:24.51 +57:39:29.5 -- not a known variable star
05:17:31.83 +57:49:59.7 -- not a known variable star
05:18:55.15 +58:43:40.0 -- a known variable star
05:19:19.08 +58:49:11.1 -- a known variable star
05:20:23.60 +58:15:45.7 -- not a known variable star
05:20:41.53 +58:47:16.6 -- not a known variable star
05:20:45.19 +59:10:52.5 -- not a known variable star
05:24:12.11 +57:31:54.1 -- a known variable star
05:24:24.61 +62:37:45.6 -- a known variable star
05:24:37.77 +57:14:43.8 -- a known variable star
05:24:42.31 +60:06:59.4 -- not a known variable star
05:25:02.32 +59:26:05.8 -- a known variable star
05:25:16.39 +58:59:13.0 -- not a known variable star
05:25:41.62 +59:44:54.0 -- a known variable star
05:25:54.62 +59:36:04.4 -- not a known variable star
05:26:21.42 +60:17:36.9 -- not a known variable star
05:27:18.39 +57:34:43.0 -- not a known variable star
05:27:56.83 +61:23:37.2 -- not a known variable star
05:28:38.93 +57:14:48.0 -- a known variable star
05:29:10.96 +60:36:41.9 -- not a known variable star
05:29:58.65 +61:00:42.8 -- not a known variable star
05:30:04.50 +59:48:06.6 -- not a known variable star
05:30:17.92 +60:13:29.3 -- not a known variable star
05:30:55.18 +60:37:14.4 -- not a known variable star
05:31:45.06 +60:52:54.3 -- a known variable star
05:31:48.36 +60:08:44.4 -- not a known variable star
05:31:48.63 +59:43:20.3 -- not a known variable star
05:31:58.29 +60:29:28.1 -- not a known variable star
05:32:22.89 +60:40:32.8 -- not a known variable star
05:32:23.46 +60:58:24.7 -- not a known variable star
05:32:25.55 +60:40:50.5 -- not a known variable star
05:33:22.20 +61:37:46.7 -- a known variable star
05:33:25.57 +59:36:24.0 -- not a known variable star
05:33:37.69 +63:19:21.7 -- a known variable star
05:34:18.58 +61:23:55.3 -- not a known variable star
05:36:07.53 +60:03:31.3 -- a known variable star
05:36:29.67 +60:26:04.3 -- a known variable star
05:36:55.58 +60:53:52.4 -- not a known variable star
05:38:55.63 +61:27:37.6 -- a known variable star
05:41:43.20 +63:49:54.5 -- not a known variable star
05:47:24.44 +62:54:04.0 -- not a known variable star
05:52:46.58 +62:41:17.9 -- a known variable star
Found 40 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
65 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 65 (excluding asteroids and hot pixels, 40 new), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461258.81266060 -observatory V36
07:46:09.62 +20:23:19.4 Mercury (-0.3mag)
11:56:01.24 -00:06:44.3 Venus (-4.3mag)
05:43:42.82 +23:32:51.1 Mars (1.3mag)
08:41:13.22 +18:47:39.6 Jupiter (-1.8mag)
00:56:32.64 +03:16:43.4 Saturn (0.6mag)
04:11:30.41 +20:56:22.4 Uranus (5.8mag)
00:16:12.49 +00:13:56.5 Neptune (7.7mag)
20:28:19.45 -23:29:26.5 Pluto (14.4mag)
02:52:29.81 +21:10:25.9 Moon (-10.3mag)
-rw-r--r-- 1 apache apache 363 Aug 6 02:35 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461258.81266060:
08:41:18.89 +18:47:15.3 Io (6.0mag)
08:41:08.58 +18:48:00.1 Europa (6.3mag)
08:41:10.99 +18:47:53.1 Ganymede (5.6mag)
08:41:00.30 +18:48:38.1 Callisto (6.7mag)
08:38:49.00 +18:45:52.9 Himalia (15.7mag)
08:41:11.87 +18:47:45.9 Thebe (16.6mag)
08:38:19.70 +18:44:47.0 Elara (17.7mag)
08:45:19.18 +18:28:01.6 Pasiphae (17.9mag)
08:44:31.67 +18:57:31.2 Carme (19.0mag)
00:56:29.94 +03:17:10.4 Titan (8.4mag)
00:56:26.71 +03:16:45.7 Rhea (9.7mag)
00:56:36.53 +03:15:06.6 Iapetus (11.1mag)
00:56:19.03 +03:16:56.9 Hyperion (14.4mag)
00:55:57.55 +03:10:09.4 Phoebe (16.5mag)
-rw-r--r-- 1 apache apache 568 Aug 6 02:35 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461258.81266060:
18:55:29.07 -23:59:48.5 JWST
17:19:17.97 +39:23:13.4 Chandra
10:12:09.33 -56:53:00.8 XMM-Newton
-rw-r--r-- 1 apache apache 96 Aug 6 02:35 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461258.81266060 -observatory V36
03:11:29.73 +17:12:56.0 17.7mag P/1996 R2 (Lagerkvist)
18:02:22.65 -34:38:21.9 14.0mag P/2010 H2 (Vales)
06:52:00.22 -68:49:51.3 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:09:18.57 +32:57:12.2 17.7mag C/2017 K2 (PANSTARRS)
03:38:00.26 +36:46:41.1 16.7mag P/2021 N1 (ZTF)
22:40:12.23 +31:33:38.0 17.3mag C/2022 E2 (ATLAS)
06:41:34.46 +26:34:26.1 16.8mag C/2022 N2 (PANSTARRS)
10:19:48.06 +28:33:20.1 17.0mag C/2022 QE78 (ATLAS)
09:27:34.78 +05:17:44.5 17.9mag C/2022 R6 (PANSTARRS)
15:12:09.97 -12:12:40.9 17.9mag P/2023 B1 (PANSTARRS)
21:13:17.57 +66:13:21.4 17.9mag C/2023 H5 (Lemmon)
15:49:48.45 -12:45:27.0 14.3mag C/2023 R1 (PANSTARRS)
08:05:56.47 +31:15:35.4 15.2mag C/2024 E1 (Wierzchos)
15:07:16.76 +15:36:57.7 17.7mag C/2024 G6 (ATLAS)
19:05:33.30 +42:58:03.8 13.7mag C/2024 J3 (ATLAS)
21:13:32.10 +49:05:05.5 17.6mag C/2024 R4 (PANSTARRS)
05:13:35.83 -12:59:33.8 15.5mag C/2024 T5 (ATLAS)
06:54:58.59 +24:29:32.1 17.9mag C/2025 J1 (Borisov)
07:29:59.44 -15:52:44.6 17.7mag C/2025 R3 (PANSTARRS)
10:30:15.01 +21:01:32.0 17.3mag C/2025 V2 (Rankin)
12:56:59.58 +02:28:34.4 17.0mag C/2025 Y1 (ATLAS)
16:03:39.52 +78:00:36.4 16.8mag C/2026 A2 (Bok)
03:06:45.31 +46:08:51.0 17.1mag C/2026 B2 (Sun-Gao)
11:45:13.25 +08:20:32.6 17.3mag A/2026 E1
21:56:12.44 -26:29:42.8 6.9mag 10P/Tempel
11:27:49.22 -03:16:54.7 16.2mag 29P/Schwassmann-Wachmann
04:36:52.20 +32:16:13.9 18.0mag 47P/Ashbrook-Jackson
11:03:47.50 +05:16:02.7 17.2mag 63P/Wild
00:54:17.79 -05:22:53.5 15.4mag 65P/Gunn
05:31:12.39 +20:43:42.9 13.7mag 78P/Gehrels
20:39:42.45 -23:18:09.6 17.8mag 84P/Giclas
02:58:49.08 +13:32:48.6 16.7mag 88P/Howell
07:50:59.70 +27:55:00.5 16.1mag 93P/Lovas
04:00:58.82 +16:07:52.1 17.6mag 112P/Urata-Niijima
05:50:09.91 +30:30:23.3 16.3mag 114P/Wiseman-Skiff
09:13:57.62 +26:58:16.7 15.0mag 123P/West-Hartley
11:39:54.69 -09:31:57.4 17.1mag 124P/Mrkos
05:33:43.84 +21:11:10.4 16.1mag 128P/Shoemaker-Holt
06:25:14.34 +18:59:31.7 17.9mag 131P/Mueller
00:03:41.10 +03:25:19.9 17.6mag 139P/Vaisala-Oterma
03:21:32.85 -19:44:42.7 14.0mag 161P/Hartley-IRAS
07:09:33.04 +37:41:43.9 15.8mag 162P/SidingSpring
15:48:23.45 +39:33:51.8 12.3mag 169P/NEAT
02:39:28.45 +09:28:39.6 17.6mag 220P/McNaught
16:40:37.78 -09:57:02.7 17.7mag 235P/LINEAR
20:23:39.72 -52:50:57.2 17.8mag 259P/Garradd
03:16:32.67 +24:21:29.3 15.4mag 260P/McNaught
06:59:36.44 +37:45:12.6 17.3mag 295P/LINEAR
15:09:52.54 +03:20:57.1 17.7mag 391P/Kowalski
08:59:08.58 +18:28:10.9 17.9mag 450P/LONEOS
-rw-r--r-- 1 apache apache 2.5K Aug 6 02:35 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
22:08:07.63 -53:03:58.90 AT2026wek 2026-08-3.82 17.17
14:51:51.34 +66:13:24.60 ASASSN-26ev 2026-08-2.15 14.02
12:06:50.79 -36:16:06.20 SN2026wgm 2026-08-1.73 15.61
16:56:36.90 -59:29:26.00 ASASSN-26er 2026-07-25.82 15.09
01:21:27.83 -10:37:05.00 SN2026vbh 2026-07-25.61 15.97
21:17:31.59 +22:25:50.90 ASASSN-26eq 2026-07-24.37 15.13
18:53:36.89 +16:56:43.60 ASASSN-26ep 2026-07-23.47 -4.06
12:18:47.98 -30:48:47.50 ASASSN-26et 2026-07-22.76 13.98
13:00:47.82 +15:42:17.60 SN2026uwk 2026-07-21.75 16.38
18:52:31.11 -32:28:00.90 ASASSN-26en 2026-07-21.77 14.63
14:42:58.01 -62:32:59.10 ASASSN-26es 2026-07-20.79 15.36
20:12:45.57 -32:53:13.00 ASASSN-26em 2026-07-20.94 16.83
18:54:24.33 -46:11:51.70 ASASSN-26eu 2026-07-20.93 14.86
03:18:56.99 -80:55:10.40 AT2026ugi 2026-07-20.03 17.12
18:43:58.40 +24:22:41.80 ASASSN-26eo 2026-07-19.36 16.16
04:50:01.03 -02:22:33.80 ASASSN-26ej 2026-07-16.17 17.02
18:34:55.28 -31:41:00.90 ASASSN-26ek 2026-07-16.24 15.73
17:07:43.61 -44:21:53.50 ASASSN-26el 2026-07-15.86 16.01
14:45:08.35 +24:13:12.30 ASASSN-26ei 2026-07-16.17 16.46
10:00:46.44 -32:36:31.10 AT 2023mhb 2026-07-14.73 16.67
14:39:37.45 -11:22:36.20 AT 2026unl 2026-07-15.27 17.11
10:49:42.57 -11:25:55.80 ASASSN-26eh 2026-07-14.72 16.58
19:33:53.06 -07:15:00.80 ASASSN-22le 2026-07-14.15 15.5
02:45:40.52 -27:55:30.30 ASASSN-26ef 2026-07-12.35 15.86
23:26:43.80 +04:42:39.70 SN 2026qtn 2026-07-12.22 16.47
02:19:17.26 +28:57:15.40 ASASSN-26ec 2026-07-11.53 2.78
18:31:15.56 -05:34:31.50 AT2026stb 2026-07-11.28 -1.29
13:36:08.24 +23:29:05.00 AT2026pjf 2026-07-10.18 -0.72
17:33:39.82 +04:22:36.70 SN2026pir 2026-07-9.86 -0.66
11:21:41.26 -50:33:36.30 ASASSN-26ed 2026-07-8.8 -1.3
23:41:42.11 +26:29:49.10 AT2026qil 2026-07-9.3 16.15
20:21:30.50 -32:03:40.10 ASASSN-26ee 2026-07-7.22 15.53
19:37:44.09 -05:35:42.80 AT2026ryu 2026-07-7.17 14.88
11:06:55.46 -04:07:04.50 AT2026qqg 2026-07-5.01 16.82
19:07:23.69 -74:13:37.30 AT2026qly 2026-07-5.02 17.31
17:57:43.80 +27:18:40.10 ASASSN-26ea 2026-07-5.07 16.67
19:59:01.43 -32:07:34.30 ASASSN-26eb 2026-07-4.97 15.52
18:46:50.35 -57:44:13.20 SN 2026qqp 2026-07-5.03 -0.92
19:17:31.69 -39:55:29.90 ASASSN-26dz 2026-07-5.14 15.91
19:14:31.37 +12:03:52.90 AT 2026rdg 2026-07-3.43 11.81
04:05:50.09 -70:24:34.40 AT 2026qpr 2026-06-30.4 15.96
13:45:37.49 -05:59:35.80 SN 2026pub 2026-06-30.09 16.01
16:41:15.63 +39:17:14.70 SN 2026pel 2026-06-26.38 16.07
10:14:40.19 -35:38:21.30 ASASSN-26dy 2026-06-25.99 15.63
14:47:21.56 -40:15:51.30 ASASSN-26dv 2026-06-23.03 14.62
13:38:49.79 -77:21:06.70 ASASSN-26dw 2026-06-23.04 16.09
00:59:27.90 +33:08:13.20 SN 2026mke 2026-06-22.39 17.13
11:10:44.73 -30:20:45.50 SN 2026nmv 2026-06-22.06 16.56
21:36:15.68 -21:19:12.50 AT2026oxh 2026-06-22.15 17.14
17:31:38.38 -56:05:51.90 ASASSN-26dx 2026-06-22.02 14.72
14:10:13.44 -38:46:46.10 AT2026pvk 2026-06-22.06 16.53
20:56:47.23 -18:31:05.20 AT2026plb 2026-06-21.31 16.4
15:44:29.68 +21:00:59.30 SN2026ore 2026-06-21.29 17.57
23:50:05.98 -14:01:41.30 AT2026oxl 2026-06-21.52 17.64
17:36:54.73 -18:10:04.20 AT2026ouj 2026-06-20.92 15.15
00:34:04.08 -30:22:09.20 AT2026ntk 2026-06-18.09 17.34
20:49:13.39 +25:17:59.20 ASASSN-26du 2026-06-15.39 15.93
23:09:30.84 +32:40:42.00 SN2026oxc 2026-06-14.35 16.83
02:02:26.67 +32:04:22.70 AT2026ovz 2026-06-14.6 15.52
21:26:28.11 -72:31:19.50 AT2026nwc 2026-06-11 17.05
17:54:57.33 +26:32:34.20 SN 2026odc 2026-06-11.23 17.62
13:55:59.94 +17:30:37.20 SN 2026nyq 2026-06-11.1 16.24
00:50:45.14 -71:38:36.90 ASASSN-26dt 2026-06-11.13 10.22
14:42:19.73 +19:11:35.60 SN2026nyp 2026-06-10.3 16.32
12:23:23.92 +12:56:43.50 SN2026mta 2026-06-8.29 16.69
12:30:18.51 +47:12:33.20 SN2026oao 2026-06-9.32 17.02
10:51:05.21 -42:28:56.60 AT2026nvf 2026-06-8.12 16.75
13:50:22.48 -07:35:00.00 SN2026npn 2026-06-8.02 17.58
00:56:07.17 +43:01:43.20 ASASSN-26dq 2026-06-7.43 13.58
01:07:49.46 +41:59:43.70 SN 2026obc 2026-06-7.43 15.15
21:11:25.22 +14:14:31.90 ASASSN-26dr 2026-06-7.24 16.24
06:21:27.06 -65:16:42.00 ASASSN-26ds 2026-06-2.97 15.02
20:07:38.15 -21:07:05.40 SN2026mho 2026-05-25.18 -1.12
11:29:42.55 +79:01:03.10 AT2026min 2026-05-24.21 16.63
11:44:33.11 -68:48:32.90 ASASSN-26no 2026-05-24.03 8.35
19:00:42.82 -48:31:01.60 ASASSN-26dp 2026-05-22.31 -3.28
14:23:56.72 -58:37:47.60 ASASSN-26dn 2026-05-20.01 14.64
11:24:54.06 +47:57:01.60 AT2026nma 2026-05-20.29 15.46
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
15:16:06.61 -79:16:32.40 ASASSN-26dm 2026-05-19.03 14.44
11:24:25.21 -59:23:19.10 ASASSN-26dl 2026-05-18.02 13.55
13:45:51.52 -53:16:01.00 ASASSN-26dk 2026-05-18.16 12.96
02:05:49.69 -30:29:09.60 ASASSN-26dh 2026-05-18.43 15.37
17:50:22.87 -39:42:33.90 ASASSN-26dj 2026-05-17.05 15.7
01:13:11.60 -33:25:16.10 ASASSN-26dg 2026-05-13.41 16.8
16:44:31.77 -27:15:18.40 AT2026mhn 2026-05-12.33 15.8
09:46:31.08 -33:41:51.00 ASASSN-26di 2026-05-12.14 14.63
21:23:11.57 -19:09:45.00 AT2026kwu 2026-05-12.26 16.9
14:20:14.30 -30:20:51.90 AT2026ktm 2026-05-12.06 17.21
14:41:39.01 -37:13:46.40 AT2026lkm 2026-05-11.18 16.89
12:59:50.45 -10:58:38.80 SN2026kep 2026-05-9.06 17.5
13:37:29.61 -29:50:30.90 AT2026lkd 2026-05-9.09 17.23
09:46:42.01 -14:52:03.60 SN2026kmo 2026-05-8.99 17.51
15:03:05.28 +22:02:03.40 AT2026lxf 2026-05-8.07 13.88
10:23:49.41 -20:57:25.30 ASASSN-26df 2026-05-8.21 16.52
22:14:40.56 +05:04:51.60 2026lda 2026-05-7.56 16.2
21:35:33.81 -14:05:16.30 ASASSN-26de 2026-05-6.29 14.51
16:21:49.13 -61:36:14.60 ASASSN-26dd 2026-05-5.15 15.93
14:26:40.22 -24:48:37.50 AT2026lig 2026-05-4.27 14.63
-rw-r--r-- 1 apache apache 5.7K Aug 6 02:34 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
00:42:51.20 +41:16:59.4 PNV J00425120+4116594 2022-10-26.135 19.3mag
12:24:25.10 +28:47:12.0 TCP J12242510+2847120 2026-05-31.6015 14.8mag
00:56:07.13 +43:01:40.6 TCP J00560713+4301406 2026-06-01.4135 12.2mag
00:42:41.64 +41:15:16.2 PNV J00424164+4115162 2026-06-02.029 17.4mag
00:42:38.68 +41:15:58.2 PNV J00423868+4115582 2026-06-05.1224 19.97Umag
19:00:42.95 -48:31:01.7 PNV J19004295-4831017 2026-05-25.0752 14.2mag
09:55:21.28 +69:02:52.6 PNV J09552128+6902526 2026-06-13.933 18.9mag
19:51:21.42 +37:06:40.0 TCP J19512142+3706400 2026-06-17.2942 16.8mag
19:57:03.87 +37:41:46.4 TCP J19570387+3741464 2026-06-18.2638 17.5mag
00:42:32.04 +41:10:28.3 PNV J00423204+4110283 2026-06-26.059 16.6mag
02:19:17.36 +28:57:15.8 TCP J02191736+2857158 2026-07-12.3549 12.5mag
00:44:56.43 +41:57:41.6 PNV J00445643+4157416 2026-07-13.8026 17.98Cmag
00:42:55.36 +41:17:27.0 PNV J00425536+4117270 2026-07-20.1813 17.7mag
20:35:43.64 +61:31:32.9 TCP J20354364+6131329 2026-07-20.5443 14.4mag
21:17:31.48 +22:25:51.0 TCP J21173148+2225510 2026-07-23.5577 14.8mag
00:41:24.04 +40:49:02.8 PNV J00412404+4049028 2026-07-25.0157 18.7mag
00:43:04.26 +41:02:28.6 PNV J00430426+4102286 2026-07-26.1512 20mag
14:51:51.40 +66:13:24.0 TCP J14515140+6613240 2026-07-29.2561 13.5mag
00:43:06.15 +41:22:08.2 PNV J00430615+4122082 2026-07-30.0085 19.4mag
00:41:33.23 +41:10:12.2 PNV J00413323+4110122 2026-08-02.8913 17.1mag
-rw-r--r-- 1 apache apache 189K Aug 6 02:34 tocp_transients_list.txt
############################################################
Truncated list of recent TNS transients from https://www.wis-tns.org/ :
09:39:31.292 -08:28:35.35 AT 2026vla 2026-02-21.40 20.65
17:07:24.157 +32:28:59.94 AT 2026vkz 2026-06-16.33 21.89
18:55:34.805 +34:42:05.78 AT 2026vky 2026-06-22.39 21.01
15:27:13.875 -10:50:21.14 AT 2026vkx 2026-06-14.35 20.55
13:36:43.476 +25:28:01.16 AT 2026vkw 2026-06-25.38 20.6
04:43:04.292 -16:08:54.64 AT 2026vkv 2026-01-12.30 21.72
04:48:25.928 -18:19:58.05 AT 2026vku 2026-01-26.25 21.35
12:55:24.686 +13:58:33.13 AT 2026vkt 2026-06-05.34 21.42
11:39:28.884 +47:23:59.43 AT 2026vks 2026-01-14.61 21.82
10:26:55.799 -14:09:20.42 AT 2026vkr 2026-01-13.55 21.98
12:26:22.284 +20:06:25.68 AT 2026vkq 2026-02-13.60 20.86
12:08:12.778 +41:30:56.83 AT 2026vkp 2026-06-15.27 20.88
05:11:50.298 -12:02:24.75 AT 2026vko 2026-02-15.23 20.49
00:35:37.087 -45:29:22.45 AT 2026vkn 2026-06-26.42 23.13
04:11:06.535 -49:23:35.67 AT 2026vkm 2026-07-09.42 22.31
23:40:19.411 -26:01:53.34 AT 2026vkl 2026-07-20.59 21.47
22:23:27.160 +00:54:32.97 AT 2026vkk 2026-07-14.55 21.17
21:14:05.875 -09:55:36.50 AT 2026vkj 2026-07-20.46 21.9
17:17:56.970 +19:09:32.22 AT 2026vki 2026-07-19.39 21.8
17:18:18.165 +24:21:20.44 AT 2026vkh 2026-07-19.40 21.78
-rw-r--r-- 1 apache apache 87K Aug 6 02:34 tns_transients_list.txt
