This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Vul-01-Q2b1x1_001133_TTUQ2b1x1_107568_dLmHE55X
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 06 08.1580 2461199.6580 12.70 19:41:34.76 +25:19:21.9
60.98044 1.17051 galactic Vul Second-epoch detections are separated by 1.6" and 9.0 pix
The object was found in ASASSN-V 2" ASASSN-V J194134.84+251924.0
Type: SR
MeanMag 14.62 m Amp. 0.14 m Period 32.7496952 d
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:41:34.76 +25:19:21.9: 13.79 +/- 0.05 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:41:34.76 +25:19:21.9: 13.83 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.04
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,2461199.6580,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260608.1580 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1580 2461199.6580 12.21 19:37:10.14 +18:11:20.2
54.26537 -1.44748 galactic Sge Second-epoch detections are separated by 2.1" and 9.5 pix
The object was found in VSX 0" ZTF J193710.13+181119.7
Type: SR
# Max. Min./Amp. JD0 Period
14.840 g Y 0.215 g 2458383.88310 48.162798900000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:37:10.14 +18:11:20.2: 13.15 +/- 0.03 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:37:10.14 +18:11:20.2: 13.17 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.16 +/- 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
ZTF J193710.13+181119.7,2461199.6580,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J193710.13+181119.7 20260608.1580 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1580 2461199.6580 11.68 19:38:48.59 +20:48:32.7
56.73945 -0.50119 galactic Vul Second-epoch detections are separated by 0.5" and 9.4 pix
The object was found in VSX 1" ASAS J193849+2048.5
Type: SR
# Max. Min./Amp. JD0 Period
9.139 Ic Y 0.359 Ic 2452589.80000 141.700000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:38:48.59 +20:48:32.7: 12.59 +/- 0.02 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:38:48.59 +20:48:32.7: 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
ASAS J193849+2048.5,2461199.6580,11.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J193849+2048.5 20260608.1580 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 06 08.1580 2461199.6580 12.34 19:41:26.52 +24:54:55.2
60.61095 0.99592 galactic Vul Second-epoch detections are separated by 2.6" and 9.3 pix
The object was found in VSX 5" ZTF J194126.88+245457.2
Type: SR
# Max. Min./Amp. JD0 Period
14.477 r Y 0.472 r 2458373.70190 173.017717200000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:41:26.52 +24:54:55.2: 13.30 +/- 0.03 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:41:26.52 +24:54:55.2: 13.32 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.31 +/- 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
ZTF J194126.88+245457.2,2461199.6580,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J194126.88+245457.2 20260608.1580 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1580 2461199.6580 12.65 19:42:23.64 +25:17:59.3
61.05176 0.99922 galactic Vul Second-epoch detections are separated by 0.5" and 9.2 pix
The object was found in VSX 4" ASASSN-V J194223.82+251802.0
Type: SR
# Max. Min./Amp. JD0 Period
14.430 V 14.640 V 2458336.72490 57.328419900000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:42:23.64 +25:17:59.3: 13.70 +/- 0.05 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:42:23.64 +25:17:59.3: 13.66 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.03
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 J194223.82+251802.0,2461199.6580,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J194223.82+251802.0 20260608.1580 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1580 2461199.6580 12.63 19:38:14.25 +21:15:17.1
57.06222 -0.16611 galactic Vul Second-epoch detections are separated by 2.9" and 9.1 pix
The object was found in VSX 2" ASAS J193814+2115.3
Type: MISC
# Max. Min./Amp. JD0 Period
9.148 Ic Y 0.638 Ic 2452654.50000 163.600000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:38:14.25 +21:15:17.1: 13.51 +/- 0.04 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:38:14.25 +21:15:17.1: 13.60 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.03
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
ASAS J193814+2115.3,2461199.6580,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J193814+2115.3 20260608.1580 12.63CV 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 06 08.1580 2461199.6580 12.47 19:37:41.06 +18:16:58.6
54.40723 -1.50829 galactic Sge Second-epoch detections are separated by 0.7" and 9.6 pix
The object was found in VSX 3" NSVS J1937405+181707
Type: SR
# Max. Min./Amp. JD0 Period
13.181 r Y 0.977 r 2458388.62100 201.706636800000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:37:41.06 +18:16:58.6: 13.78 +/- 0.06 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:37:41.06 +18:16:58.6: 13.95 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.85 +/- 0.05
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 J1937405+181707,2461199.6580,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J1937405+181707 20260608.1580 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1580 2461199.6580 12.13 19:36:57.34 +24:15:05.0
59.53125 1.55795 galactic Vul Second-epoch detections are separated by 1.2" and 9.2 pix
The object was found in VSX 4" ASASSN-V J193657.55+241508.3
Type: L:
# Max. Min./Amp. JD0 Period
13.570 V 14.200 V
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:36:57.34 +24:15:05.0: 13.04 +/- 0.03 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:36:57.34 +24:15:05.0: 13.10 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.07 +/- 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 J193657.55+241508.3,2461199.6580,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J193657.55+241508.3 20260608.1580 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1580 2461199.6580 13.14 19:38:31.88 +20:59:27.0
56.86586 -0.35529 galactic Vul Second-epoch detections are separated by 0.4" and 9.5 pix
The object was found in VSX 3" Gaia DR3 1826041256144654848
Type: VAR
# Max. Min./Amp. JD0 Period
12.970 G 13.000 G 0.022971500000 C
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:38:31.88 +20:59:27.0: 14.27 +/- 0.07 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:38:31.88 +20:59:27.0: 14.17 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.22 +/- 0.05
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 1826041256144654848,2461199.6580,13.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1826041256144654848 20260608.1580 13.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1580 2461199.6580 12.94 19:40:57.01 +25:16:36.9
60.87027 1.27146 galactic Vul Second-epoch detections are separated by 2.2" and 9.7 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 | 19:40:57.01 +25:16:36.9 (user input) | T | P | (position from user input) J-Ks=1.447+/-0.028 (Very red! L if it's a dwarf)
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:40:57.01 +25:16:36.9: 14.07 +/- 0.06 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:40:57.01 +25:16:36.9: 14.11 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.09 +/- 0.05
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,2461199.6580,12.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1580 12.94CV 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 06 08.1580 2461199.6580 13.02 19:35:05.65 +19:23:07.6
55.07104 -0.43563 galactic Sge Second-epoch detections are separated by 1.8" and 9.2 pix
The object was found in VSX 1" ASASSN-V J193505.67+192308.2
Type: SRS
# Max. Min./Amp. JD0 Period
14.460 V 14.540 V 2457174.09400 14.909000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:35:05.65 +19:23:07.6: 13.96 +/- 0.06 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:35:05.65 +19:23:07.6: 14.05 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.00 +/- 0.04
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 J193505.67+192308.2,2461199.6580,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J193505.67+192308.2 20260608.1580 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1580 2461199.6580 12.58 19:40:37.60 +25:48:06.4
61.29086 1.59398 galactic Vul Second-epoch detections are separated by 0.8" and 9.2 pix
The object was found in VSX 5" NSVS J1940382+254812
Type: M
# Max. Min./Amp. JD0 Period
13.776 r Y 2.524 r 2458233.70720 169.479105900000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:40:37.60 +25:48:06.4: 13.61 +/- 0.05 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:40:37.60 +25:48:06.4: 13.47 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.53 +/- 0.03
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 J1940382+254812,2461199.6580,12.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J1940382+254812 20260608.1580 12.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1580 2461199.6580 12.89 19:39:36.46 +25:05:22.4
60.55746 1.44338 galactic Vul Second-epoch detections are separated by 2.4" and 9.3 pix
The object was found in VSX 3" ASASSN-V J193936.59+250525.2
Type: SR
# Max. Min./Amp. JD0 Period
14.320 V 14.440 V 2458002.89000 36.850000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:39:36.46 +25:05:22.4: 13.93 +/- 0.07 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:39:36.46 +25:05:22.4: 13.87 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.90 +/- 0.05
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 J193936.59+250525.2,2461199.6580,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J193936.59+250525.2 20260608.1580 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1580 2461199.6580 12.86 19:39:30.68 +24:11:42.3
59.76774 1.02244 galactic Vul Second-epoch detections are separated by 1.2" and 9.3 pix
The object was found in VSX 8" Gaia DR3 2020389900667180032
Type: L
# Max. Min./Amp. JD0 Period
18.320 G 18.600 G
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:39:30.68 +24:11:42.3: 13.84 +/- 0.06 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:39:30.68 +24:11:42.3: 13.89 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.86 +/- 0.04
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 2020389900667180032,2461199.6580,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2020389900667180032 20260608.1580 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1580 2461199.6580 12.04 19:41:49.55 +26:10:35.6
61.75001 1.54488 galactic Vul Second-epoch detections are separated by 1.8" and 9.0 pix
The object was found in VSX 9" NSVS J1941500+261042
Type: L:
# Max. Min./Amp. JD0 Period
10.919 R1 Y 0.337 R1 171.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:41:49.55 +26:10:35.6: 12.99 +/- 0.03 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:41:49.55 +26:10:35.6: 12.93 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.96 +/- 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
NSVS J1941500+261042,2461199.6580,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J1941500+261042 20260608.1580 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 06 08.1580 2461199.6580 12.40 19:41:34.34 +25:11:40.8
60.86833 1.10850 galactic Vul Second-epoch detections are separated by 2.0" and 9.0 pix
The object was found in VSX 3" ASASSN-V J194134.38+251143.4
Type: SR
# Max. Min./Amp. JD0 Period
14.190 V 14.340 V 2458315.94000 41.750000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:41:34.34 +25:11:40.8: 13.39 +/- 0.04 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:41:34.34 +25:11:40.8: 13.34 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.03
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 J194134.38+251143.4,2461199.6580,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J194134.38+251143.4 20260608.1580 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1580 2461199.6580 12.99 19:37:29.72 +23:30:37.9
58.94495 1.08834 galactic Vul Second-epoch detections are separated by 2.1" and 8.9 pix
The object was found in VSX 5" NSVS J1937293+233034
Type: M
# Max. Min./Amp. JD0 Period
17.258 g Y 5.425 g 2458272.91770 231.111449100000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:37:29.72 +23:30:37.9: 14.71 +/- 0.13 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:37:29.72 +23:30:37.9: 14.65 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.68 +/- 0.09
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 J1937293+233034,2461199.6580,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J1937293+233034 20260608.1580 12.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1580 2461199.6580 12.64 19:38:56.89 +24:13:03.4
59.72423 1.14534 galactic Vul Second-epoch detections are separated by 1.2" and 9.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2021141279460690688 | 19:38:56.98 +24:13:05.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.422+/-0.032 (Very red! L if it's a dwarf)
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:38:56.89 +24:13:03.4: 13.57 +/- 0.04 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:38:56.89 +24:13:03.4: 13.59 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.58 +/- 0.03
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 2021141279460690688,2461199.6580,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2021141279460690688 20260608.1580 12.64CV 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 06 08.1580 2461199.6580 12.71 19:41:54.35 +25:38:48.8
61.29861 1.26698 galactic Vul Second-epoch detections are separated by 3.5" and 9.7 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 | 19:41:54.35 +25:38:48.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:41:54.35 +25:38:48.8: 13.74 +/- 0.05 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:41:54.35 +25:38:48.8: 13.62 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.03
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,2461199.6580,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1580 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1580 2461199.6580 12.79 18:55:20.32 +25:41:34.4
56.48960 10.60523 galactic Her Second-epoch detections are separated by 4.6" and 8.0 pix
The object was found in VSX 3" ASASSN-V J185520.32+254138.0
Type: SR
# Max. Min./Amp. JD0 Period
13.940 V 14.710 V 2458373.38670 91.088807300000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 18:55:20.32 +25:41:34.4: 13.97 +/- 0.08 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 18:55:20.32 +25:41:34.4: 13.84 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.90 +/- 0.05
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!
TCP 2026 06 08.1580* 18 55 20.32 +25 41 34.4 12.8 U Her 9 0
Don'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 J185520.32+254138.0,2461199.6580,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J185520.32+254138.0 20260608.1580 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1580 2461199.6580 12.87 19:37:10.54 +18:20:09.9
54.39458 -1.37699 galactic Sge Second-epoch detections are separated by 0.8" and 9.6 pix
The object was found in VSX 2" ASASSN-V J193710.63+182008.8
Type: SR
# Max. Min./Amp. JD0 Period
14.990 V 15.700 V 2458586.62770 180.845661900000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:37:10.54 +18:20:09.9: 13.84 +/- 0.06 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:37:10.54 +18:20:09.9: 13.79 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.82 +/- 0.04
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 J193710.63+182008.8,2461199.6580,12.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J193710.63+182008.8 20260608.1580 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1580 2461199.6580 12.71 19:39:40.24 +23:47:34.9
59.43560 0.79290 galactic Vul Second-epoch detections are separated by 1.6" and 9.4 pix
The object was found in VSX 3" ASASSN-V J193940.31+234737.6
Type: SR
# Max. Min./Amp. JD0 Period
14.360 V 14.730 V 2457661.70000 62.600000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:39:40.24 +23:47:34.9: 13.79 +/- 0.06 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:39:40.24 +23:47:34.9: 13.73 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.76 +/- 0.04
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 J193940.31+234737.6,2461199.6580,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J193940.31+234737.6 20260608.1580 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1580 2461199.6580 12.42 19:38:41.68 +18:20:16.3
54.57261 -1.69047 galactic Sge Second-epoch detections are separated by 2.6" and 10.0 pix
The object was found in VSX 1" NSVS 11256648
Type: SR
# Max. Min./Amp. JD0 Period
13.346 r Y 0.677 r 2458268.91220 89.200945000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:38:41.68 +18:20:16.3: 13.59 +/- 0.05 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:38:41.68 +18:20:16.3: 13.50 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.54 +/- 0.03
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 11256648,2461199.6580,12.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 11256648 20260608.1580 12.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1580 2461199.6580 12.62 19:42:10.71 +25:14:36.2
60.97859 1.01354 galactic Vul Second-epoch detections are separated by 0.7" and 9.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:42:10.71 +25:14:36.2 (user input) | T | P | (position from user input) J-Ks=0.687+/-0.028 (K)
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:42:10.71 +25:14:36.2: 13.53 +/- 0.04 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:42:10.71 +25:14:36.2: 13.61 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.03
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,2461199.6580,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1580 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1580 2461199.6580 12.45 19:38:57.41 +23:32:12.4
59.13207 0.80920 galactic Vul Second-epoch detections are separated by 1.7" and 9.1 pix
The object was found in VSX 2" ASASSN-V J193857.53+233212.5
Type: SR
# Max. Min./Amp. JD0 Period
14.370 V 14.980 V 2458374.99380 87.173248800000
The object was not found in astcheck.
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:38:57.41 +23:32:12.4: 13.83 +/- 0.07 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:38:57.41 +23:32:12.4: 13.85 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.84 +/- 0.05
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 J193857.53+233212.5,2461199.6580,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J193857.53+233212.5 20260608.1580 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461177.93408543 17.05.2026 10:24:54.981 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits
First image: 2461177.93408543 17.05.2026 10:24:54.981 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits
Last image: 2461199.65837444 08.06.2026 03:47:53.552 /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Vul-01-Q2b1x1_001133_TTUQ2b1x1_107568_dLmHE55X/fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.67
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 6 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 17561
Objects passed selection criteria: 17458
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 12075.5
Average stars matched: 11740 (97.2216 %)
Memory usage VmPeak: 124736 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Jun 7 22:21:29 CDT 2026
VaST build number 1.0rc89-90-g333d5534
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-07)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Jun 8 00:14:02 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: 2461177.93408543 17.05.2026 10:24:54.981 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits
First image: 2461177.93408543 17.05.2026 10:24:54.981 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits
Last image: 2461199.65837444 08.06.2026 03:47:53.552 /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Vul-01-Q2b1x1_001133_TTUQ2b1x1_107568_dLmHE55X/fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 154
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.32
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: 57 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 163841
Objects passed selection criteria: 163423
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 118707
Average stars matched: 113462 (95.5813 %)
Memory usage VmPeak: 2005224 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Jun 7 22:21:29 CDT 2026
VaST build number 1.0rc89-90-g333d5534
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-07)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Jun 8 00:20:23 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Vul-01-Q2b1x1_001133_TTUQ2b1x1_107568_dLmHE55X/fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Vul-01-Q2b1x1_001133_TTUQ2b1x1_107568_dLmHE55X/fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits
SExtractor catalog cache: saved Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits.cat to cache
SExtractor catalog cache: saved Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.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/Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Vul-01-Q2b1x1_001133_TTUQ2b1x1_107568_dLmHE55X/fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Vul-01-Q2b1x1_001133_TTUQ2b1x1_107568_dLmHE55X/fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.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: 2461199.65770866
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits exists and is non-empty
Saving wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits to local_wcs_cache/
'wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits' -> 'local_wcs_cache/wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits'
wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits exists and is non-empty
Saving wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits to local_wcs_cache/
'wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits' -> 'local_wcs_cache/wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits'
wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits exists and is non-empty
Saving wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits to local_wcs_cache/
'wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits' -> 'local_wcs_cache/wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits'
wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits exists and is non-empty
Saving wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits to local_wcs_cache/
'wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits' -> 'local_wcs_cache/wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits (1st reference image)
verification OK: wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits
Image size: 937.2'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 19:23:04.854 +22:00:37.73 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits (1st new image)
verification OK: wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits
Image size: 938.7'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 19:23:27.415 +22:00:25.70 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 19:23:04.854 +22:00:37.73
Second-epoch image center 19:23:27.415 +22:00:25.70
Angular distance between the image centers 0.0872 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits (2nd new image)
verification OK: wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits
Image size: 938.6'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 19:23:24.688 +21:59:47.99 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 19:23:04.854 +22:00:37.73
Second-epoch image center 19:23:24.688 +21:59:47.99
Angular distance between the image centers 0.0779 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 19:23:27.415 +22:00:25.70
Second-epoch second image center 19:23:24.688 +21:59:47.99
Angular distance between the image centers 0.01486 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits &> /tmp/tmp.LIg3CdQm2h
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits &> /tmp/tmp.yQ9IoRbM7s
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Vul-01-Q2b1x1_001133_TTUQ2b1x1_107568_dLmHE55X/fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits &> /tmp/tmp.o8uWNrXsJG
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Vul-01-Q2b1x1_001133_TTUQ2b1x1_107568_dLmHE55X/fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Vul-01-Q2b1x1_001133_TTUQ2b1x1_107568_dLmHE55X/fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits &> /tmp/tmp.82CEzyxyz2
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Vul-01-Q2b1x1_001133_TTUQ2b1x1_107568_dLmHE55X/fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits
Calibrating the magnitude scale
Found non-empty wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.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_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits and wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits.cat
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_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits and wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits.cat
Found non-empty wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits and wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits.cat
The reference image (wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits) and catalog (wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits.cat) found
'wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits.cat' -> 'wcsmag.cat'
Read 27697 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 282.0096 to 299.5216 deg, Dec +16.5872 to +27.2740 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 282.0096 to 299.5216 deg, Dec 16.5872 to 27.2740 deg
Loaded 18852 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): 12639 out of 13800 total matches.
Matched with Tycho-2 13800 out of 27697 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.736400
a=0.000000 b=1.000000 c=22.736400
From vast_summary.log: estimated ref. image limiting mag.: -7.67
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.07
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.07
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 27697 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 282.0096 to 299.5216 deg, Dec +16.5872 to +27.2740 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 282.0096 to 299.5216 deg, Dec 16.5872 to 27.2740 deg
Loaded 18852 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): 12639 out of 13800 total matches.
Matched with Tycho-2 13800 out of 27697 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits:
Forced-photometry filter: calibrated wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits -> calib.txt_param_ref_wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits (aperture=6.2)
Read 27510 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 282.0087 to 299.5187 deg, Dec +16.5999 to +27.2874 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 282.0087 to 299.5187 deg, Dec 16.5999 to 27.2874 deg
Loaded 18870 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): 13183 out of 14382 total matches.
Matched with Tycho-2 14382 out of 27510 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits:
Forced-photometry filter: calibrated wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits -> calib.txt_param_ref_wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits (aperture=6.2)
____ 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: 8000)
Median FWHM seeing for isolated stars:
2.4 pix Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits
2.4 pix Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits
2.7 pix fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits
2.7 pix fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits
2.4 pix wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits
2.4 pix wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits
Limiting magnitude estimates:
15.1 mag. Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits
15.1 mag. Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits
13.5 mag. fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits
13.7 mag. fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits
All-image limiting magnitude estimate: 13.5 (SNR ) 11.0 (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 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.LIg3CdQm2h (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_2026-06-08_CI_Vul-01-Q2b1x1_001133_TTUQ2b1x1_107568_dLmHE55X/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits' -> 'wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits
WCS_IMAGE_NAME=wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits
WCS-calibrated image found: wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits
Checking if the catalog wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits.cat corresponding to the image wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits alredy exist and is non-empty...
Catalog wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits.cat corresponding to the image wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits
WCS catalog name: wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2722, passed=27697
Got 27697 stars (including 24942 good ones) from the SExtractor catalog wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits.cat
util/solve_plate_with_UCAC5 got 27697 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 950 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.75"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 27171 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.84"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 27170 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.84"
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 27170 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.83"
Excluding outliers - 961 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits N_match=961 sigma_overall_arcsec=0.788 sigma_q1_arcsec=0.667 sigma_q2_arcsec=0.951 sigma_q3_arcsec=0.641 sigma_q4_arcsec=0.778 n_q1=188 n_q2=306 n_q3=188 n_q4=279 worst_quadrant_to_overall_ratio=1.207
The image catalog is written to wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits -region wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.yQ9IoRbM7s (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_2026-06-08_CI_Vul-01-Q2b1x1_001133_TTUQ2b1x1_107568_dLmHE55X/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits' -> 'wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits
WCS_IMAGE_NAME=wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits
WCS-calibrated image found: wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits
Checking if the catalog wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits.cat corresponding to the image wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits alredy exist and is non-empty...
Catalog wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits.cat corresponding to the image wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits
WCS catalog name: wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits.cat
SExtractor catalog parsing summary: zero_flux=4, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2737, passed=27506
Got 27506 stars (including 24749 good ones) from the SExtractor catalog wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits.cat
util/solve_plate_with_UCAC5 got 27506 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 953 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 27007 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.75"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 27007 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.75"
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 27006 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.80"
Excluding outliers - 960 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits N_match=960 sigma_overall_arcsec=0.747 sigma_q1_arcsec=0.699 sigma_q2_arcsec=0.901 sigma_q3_arcsec=0.615 sigma_q4_arcsec=0.714 n_q1=186 n_q2=307 n_q3=193 n_q4=274 worst_quadrant_to_overall_ratio=1.206
The image catalog is written to wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits -region wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.o8uWNrXsJG (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_2026-06-08_CI_Vul-01-Q2b1x1_001133_TTUQ2b1x1_107568_dLmHE55X/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Vul-01-Q2b1x1_001133_TTUQ2b1x1_107568_dLmHE55X/fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Vul-01-Q2b1x1_001133_TTUQ2b1x1_107568_dLmHE55X/fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Vul-01-Q2b1x1_001133_TTUQ2b1x1_107568_dLmHE55X/fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Vul-01-Q2b1x1_001133_TTUQ2b1x1_107568_dLmHE55X/fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Vul-01-Q2b1x1_001133_TTUQ2b1x1_107568_dLmHE55X/fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.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_2026-06-08_CI_Vul-01-Q2b1x1_001133_TTUQ2b1x1_107568_dLmHE55X/fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits
WCS_IMAGE_NAME=wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits
WCS-calibrated image found: wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits
Checking if the catalog wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits.cat corresponding to the image wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits alredy exist and is non-empty...
Catalog wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits.cat corresponding to the image wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Vul-01-Q2b1x1_001133_TTUQ2b1x1_107568_dLmHE55X/fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits
WCS catalog name: wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=458, passed=8878
Got 8878 stars (including 8415 good ones) from the SExtractor catalog wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits.cat
util/solve_plate_with_UCAC5 got 8878 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.7'
Seting catalog search parameters based on the expected field of view 938.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013038 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010430 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 922 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 8596 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.75"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 8597 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.76"
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 8597 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.86"
Excluding outliers - 950 stars left (next iteration limit 1045)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits N_match=950 sigma_overall_arcsec=0.826 sigma_q1_arcsec=0.677 sigma_q2_arcsec=0.803 sigma_q3_arcsec=0.785 sigma_q4_arcsec=0.988 n_q1=149 n_q2=342 n_q3=138 n_q4=321 worst_quadrant_to_overall_ratio=1.197
The image catalog is written to wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Vul-01-Q2b1x1_001133_TTUQ2b1x1_107568_dLmHE55X/fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits -region wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.82CEzyxyz2 (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_2026-06-08_CI_Vul-01-Q2b1x1_001133_TTUQ2b1x1_107568_dLmHE55X/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Vul-01-Q2b1x1_001133_TTUQ2b1x1_107568_dLmHE55X/fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Vul-01-Q2b1x1_001133_TTUQ2b1x1_107568_dLmHE55X/fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Vul-01-Q2b1x1_001133_TTUQ2b1x1_107568_dLmHE55X/fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Vul-01-Q2b1x1_001133_TTUQ2b1x1_107568_dLmHE55X/fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Vul-01-Q2b1x1_001133_TTUQ2b1x1_107568_dLmHE55X/fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.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_2026-06-08_CI_Vul-01-Q2b1x1_001133_TTUQ2b1x1_107568_dLmHE55X/fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits
WCS_IMAGE_NAME=wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits
WCS-calibrated image found: wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits
Checking if the catalog wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits.cat corresponding to the image wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits alredy exist and is non-empty...
Catalog wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits.cat corresponding to the image wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Vul-01-Q2b1x1_001133_TTUQ2b1x1_107568_dLmHE55X/fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits
WCS catalog name: wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=440, passed=8746
Got 8746 stars (including 8300 good ones) from the SExtractor catalog wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits.cat
util/solve_plate_with_UCAC5 got 8746 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.6'
Seting catalog search parameters based on the expected field of view 938.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013036 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010429 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 923 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.77"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 8536 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.83"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 8533 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.85"
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 8531 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.00"
Excluding outliers - 947 stars left (next iteration limit 1041)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits N_match=947 sigma_overall_arcsec=0.919 sigma_q1_arcsec=0.752 sigma_q2_arcsec=1.028 sigma_q3_arcsec=0.703 sigma_q4_arcsec=1.145 n_q1=159 n_q2=320 n_q3=172 n_q4=296 worst_quadrant_to_overall_ratio=1.246
The image catalog is written to wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Vul-01-Q2b1x1_001133_TTUQ2b1x1_107568_dLmHE55X/fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits -region wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits.cat.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=Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits sigma_overall=0.788 worst_q_ratio=1.207
ref2=Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits sigma_overall=0.747 worst_q_ratio=1.206
new1=fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits sigma_overall=0.826 worst_q_ratio=1.197
new2=fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits sigma_overall=0.919 worst_q_ratio=1.246
reference average sigma_overall=0.7675 worst_q_ratio=1.2065
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: numpy/matplotlib unavailable (No module named 'matplotlib') -- falling back to the C plotter
plot_astrometric_residuals_xy: wrote wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311_astrometric_residuals.png (961 matched stars from wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy.py: numpy/matplotlib unavailable (No module named 'matplotlib') -- falling back to the C plotter
plot_astrometric_residuals_xy: wrote wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312_astrometric_residuals.png (960 matched stars from wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy.py: numpy/matplotlib unavailable (No module named 'matplotlib') -- falling back to the C plotter
plot_astrometric_residuals_xy: PGPLOT /PNG device reported success but no file appeared at wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070_astrometric_residuals.png -- no plot produced
WARNING: no astrometric residual plot produced for wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits -- both lib/plot_astrometric_residuals_xy.py and lib/plot_astrometric_residuals_xy failed to create wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070_astrometric_residuals.png (see messages above)
plot_astrometric_residuals_xy.py: numpy/matplotlib unavailable (No module named 'matplotlib') -- falling back to the C plotter
plot_astrometric_residuals_xy: PGPLOT /PNG device reported success but no file appeared at wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071_astrometric_residuals.png -- no plot produced
WARNING: no astrometric residual plot produced for wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits -- both lib/plot_astrometric_residuals_xy.py and lib/plot_astrometric_residuals_xy failed to create wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071_astrometric_residuals.png (see messages above)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Vul-01-Q2b1x1_001133_TTUQ2b1x1_107568_dLmHE55X/wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits'
Saving fully-calibrated image wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Vul-01-Q2b1x1_001133_TTUQ2b1x1_107568_dLmHE55X/wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits'
Preparing the HTML report for the field Vul-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Vul-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Vul-01-Q2b1x1_001133_TTUQ2b1x1_107568_dLmHE55X/fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Vul-01-Q2b1x1_001133_TTUQ2b1x1_107568_dLmHE55X/fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits
SExtractor catalog cache: saved Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits.cat to cache
SExtractor catalog cache: saved Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Vul-01-Q2b1x1_001133_TTUQ2b1x1_107568_dLmHE55X/fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Vul-01-Q2b1x1_001133_TTUQ2b1x1_107568_dLmHE55X/fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits
Creating symlink local_wcs_cache/wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits
Creating symlink local_wcs_cache/wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits
Creating symlink local_wcs_cache/wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.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_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits exists and is non-empty
wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits exists and is non-empty
wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits exists and is non-empty
wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits (1st reference image)
verification OK: wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits
Image size: 937.2'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 19:23:04.854 +22:00:37.73 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits (1st new image)
verification OK: wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits
Image size: 938.7'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 19:23:27.415 +22:00:25.70 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 19:23:04.854 +22:00:37.73
Second-epoch image center 19:23:27.415 +22:00:25.70
Angular distance between the image centers 0.0872 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits (2nd new image)
verification OK: wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits
Image size: 938.6'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 19:23:24.688 +21:59:47.99 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 19:23:04.854 +22:00:37.73
Second-epoch image center 19:23:24.688 +21:59:47.99
Angular distance between the image centers 0.0779 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 19:23:27.415 +22:00:25.70
Second-epoch second image center 19:23:24.688 +21:59:47.99
Angular distance between the image centers 0.01486 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits &> /tmp/tmp.zfYgU3wBA9
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits &> /tmp/tmp.u8dJ0DcUuG
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Vul-01-Q2b1x1_001133_TTUQ2b1x1_107568_dLmHE55X/fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits &> /tmp/tmp.ixy8zCbSHm
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Vul-01-Q2b1x1_001133_TTUQ2b1x1_107568_dLmHE55X/fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Vul-01-Q2b1x1_001133_TTUQ2b1x1_107568_dLmHE55X/fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits &> /tmp/tmp.O67wFf5CoW
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Vul-01-Q2b1x1_001133_TTUQ2b1x1_107568_dLmHE55X/fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits
Calibrating the magnitude scale
Found non-empty wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.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_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits and wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits.cat
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_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits and wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits.cat
Found non-empty wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits and wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits.cat
The reference image (wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits) and catalog (wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits.cat) found
'wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits.cat' -> 'wcsmag.cat'
Read 231758 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 281.9830 to 299.5234 deg, Dec +16.5833 to +27.2757 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 281.9830 to 299.5234 deg, Dec 16.5833 to 27.2757 deg
Loaded 18886 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): 9948 out of 14403 total matches.
Matched with Tycho-2 14403 out of 231758 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.573700
a=0.000000 b=1.000000 c=22.573700
From vast_summary.log: estimated ref. image limiting mag.: -7.32
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.25
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.25
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 231758 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 281.9830 to 299.5234 deg, Dec +16.5833 to +27.2757 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 281.9830 to 299.5234 deg, Dec 16.5833 to 27.2757 deg
Loaded 18886 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): 9948 out of 14403 total matches.
Matched with Tycho-2 14403 out of 231758 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits:
Forced-photometry filter: calibrated wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits -> calib.txt_param_ref_wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits (aperture=4.6)
Read 231606 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 281.9803 to 299.5194 deg, Dec +16.5979 to +27.2882 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 281.9803 to 299.5194 deg, Dec 16.5979 to 27.2882 deg
Loaded 18902 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): 10347 out of 15024 total matches.
Matched with Tycho-2 15024 out of 231606 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits:
Forced-photometry filter: calibrated wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits -> calib.txt_param_ref_wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits (aperture=4.5)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 105 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.2 pix Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits
2.2 pix Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits
2.4 pix fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits
2.4 pix fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits
2.2 pix wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits
2.2 pix wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits
Limiting magnitude estimates:
15.3 mag. Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits
15.2 mag. Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits
13.6 mag. fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits
13.6 mag. fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits
All-image limiting magnitude estimate: 13.6 (SNR ) 13.2 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.zfYgU3wBA9 (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_2026-06-08_CI_Vul-01-Q2b1x1_001133_TTUQ2b1x1_107568_dLmHE55X/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits' -> 'wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits
WCS_IMAGE_NAME=wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits
WCS-calibrated image found: wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits
Checking if the catalog wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits.cat corresponding to the image wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits alredy exist and is non-empty...
Catalog wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits.cat corresponding to the image wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits
WCS catalog name: wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=36, blended=36344, passed=231722
Got 231722 stars (including 195045 good ones) from the SExtractor catalog wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits.cat
util/solve_plate_with_UCAC5 got 231722 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 949 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 226904 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 226905 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 226904 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Excluding outliers - 959 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits N_match=959 sigma_overall_arcsec=0.716 sigma_q1_arcsec=0.632 sigma_q2_arcsec=0.809 sigma_q3_arcsec=0.613 sigma_q4_arcsec=0.674 n_q1=203 n_q2=292 n_q3=182 n_q4=282 worst_quadrant_to_overall_ratio=1.130
The image catalog is written to wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits -region wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.u8dJ0DcUuG (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_2026-06-08_CI_Vul-01-Q2b1x1_001133_TTUQ2b1x1_107568_dLmHE55X/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits' -> 'wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits
WCS_IMAGE_NAME=wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits
WCS-calibrated image found: wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits
Checking if the catalog wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits.cat corresponding to the image wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits alredy exist and is non-empty...
Catalog wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits.cat corresponding to the image wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits
WCS catalog name: wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits.cat
SExtractor catalog parsing summary: zero_flux=10, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=32, blended=36086, passed=231564
Got 231564 stars (including 195178 good ones) from the SExtractor catalog wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits.cat
util/solve_plate_with_UCAC5 got 231564 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 948 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 225736 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 225734 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 225733 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Excluding outliers - 959 stars left (next iteration limit 1054)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits N_match=959 sigma_overall_arcsec=0.704 sigma_q1_arcsec=0.606 sigma_q2_arcsec=0.755 sigma_q3_arcsec=0.575 sigma_q4_arcsec=0.669 n_q1=205 n_q2=289 n_q3=184 n_q4=281 worst_quadrant_to_overall_ratio=1.073
The image catalog is written to wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits -region wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.ixy8zCbSHm (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_2026-06-08_CI_Vul-01-Q2b1x1_001133_TTUQ2b1x1_107568_dLmHE55X/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Vul-01-Q2b1x1_001133_TTUQ2b1x1_107568_dLmHE55X/fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Vul-01-Q2b1x1_001133_TTUQ2b1x1_107568_dLmHE55X/fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Vul-01-Q2b1x1_001133_TTUQ2b1x1_107568_dLmHE55X/fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Vul-01-Q2b1x1_001133_TTUQ2b1x1_107568_dLmHE55X/fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Vul-01-Q2b1x1_001133_TTUQ2b1x1_107568_dLmHE55X/fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.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_2026-06-08_CI_Vul-01-Q2b1x1_001133_TTUQ2b1x1_107568_dLmHE55X/fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits
WCS_IMAGE_NAME=wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits
WCS-calibrated image found: wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits
Checking if the catalog wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits.cat corresponding to the image wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits alredy exist and is non-empty...
Catalog wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits.cat corresponding to the image wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Vul-01-Q2b1x1_001133_TTUQ2b1x1_107568_dLmHE55X/fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits
WCS catalog name: wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=4743, passed=73672
Got 73672 stars (including 68816 good ones) from the SExtractor catalog wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits.cat
util/solve_plate_with_UCAC5 got 73672 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.7'
Seting catalog search parameters based on the expected field of view 938.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013038 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010430 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 926 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 71813 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 71814 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 71814 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Excluding outliers - 954 stars left (next iteration limit 1049)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits N_match=954 sigma_overall_arcsec=0.788 sigma_q1_arcsec=0.661 sigma_q2_arcsec=0.782 sigma_q3_arcsec=0.698 sigma_q4_arcsec=0.856 n_q1=164 n_q2=323 n_q3=155 n_q4=312 worst_quadrant_to_overall_ratio=1.086
The image catalog is written to wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Vul-01-Q2b1x1_001133_TTUQ2b1x1_107568_dLmHE55X/fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits -region wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.O67wFf5CoW (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_2026-06-08_CI_Vul-01-Q2b1x1_001133_TTUQ2b1x1_107568_dLmHE55X/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Vul-01-Q2b1x1_001133_TTUQ2b1x1_107568_dLmHE55X/fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Vul-01-Q2b1x1_001133_TTUQ2b1x1_107568_dLmHE55X/fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Vul-01-Q2b1x1_001133_TTUQ2b1x1_107568_dLmHE55X/fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Vul-01-Q2b1x1_001133_TTUQ2b1x1_107568_dLmHE55X/fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Vul-01-Q2b1x1_001133_TTUQ2b1x1_107568_dLmHE55X/fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.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_2026-06-08_CI_Vul-01-Q2b1x1_001133_TTUQ2b1x1_107568_dLmHE55X/fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits
WCS_IMAGE_NAME=wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits
WCS-calibrated image found: wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits
Checking if the catalog wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits.cat corresponding to the image wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits alredy exist and is non-empty...
Catalog wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits.cat corresponding to the image wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Vul-01-Q2b1x1_001133_TTUQ2b1x1_107568_dLmHE55X/fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits
WCS catalog name: wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=4767, passed=73028
Got 73028 stars (including 68159 good ones) from the SExtractor catalog wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits.cat
util/solve_plate_with_UCAC5 got 73028 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.6'
Seting catalog search parameters based on the expected field of view 938.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013036 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010429 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 933 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 71205 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 71205 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 71203 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.74"
Excluding outliers - 954 stars left (next iteration limit 1049)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits N_match=954 sigma_overall_arcsec=0.814 sigma_q1_arcsec=0.698 sigma_q2_arcsec=0.882 sigma_q3_arcsec=0.708 sigma_q4_arcsec=0.993 n_q1=182 n_q2=296 n_q3=178 n_q4=298 worst_quadrant_to_overall_ratio=1.219
The image catalog is written to wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Vul-01-Q2b1x1_001133_TTUQ2b1x1_107568_dLmHE55X/fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits -region wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits.cat.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_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.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_2026-06-08_CI_Vul-01-Q2b1x1_001133_TTUQ2b1x1_107568_dLmHE55X/wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-46-56_20.00sec_5.00C_LIGHT_0070.fits
Saving fully-calibrated image wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.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_2026-06-08_CI_Vul-01-Q2b1x1_001133_TTUQ2b1x1_107568_dLmHE55X/wcs_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071.fits
Preparing the HTML report for the field Vul-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 18:58:27.49 +19:40:52.0: 13.10 +/- 0.03 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:37:54.84 +23:46:57.5: 12.98 +/- 0.03 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:35:48.34 +17:49:57.4: 13.38 +/- 0.04 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:29:56.90 +18:21:41.8: 13.18 +/- 0.03 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:17:53.38 +22:36:07.9: 12.42 +/- 0.01 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:11:49.32 +20:10:48.5: 13.13 +/- 0.03 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:41:43.73 +18:59:40.4: 13.27 +/- 0.04 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 18:54:19.05 +24:53:11.0: 13.75 +/- 0.06 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:01:42.64 +20:46:56.7: 12.93 +/- 0.03 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 18:58:27.49 +19:40:52.0: 13.10 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.02
Forced photometry filter REJECTED candidate at 18:58:27.49 +19:40:52.0: ref_mag=13.10 +/- 0.02 new_mean_mag=12.9343 delta=0.17 (need > 0.90)
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:37:54.84 +23:46:57.5: 13.03 +/- 0.03 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:29:56.90 +18:21:41.8: 13.23 +/- 0.03 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:17:53.38 +22:36:07.9: 12.48 +/- 0.01 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.02
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:35:48.34 +17:49:57.4: 13.35 +/- 0.04 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:11:49.32 +20:10:48.5: 13.14 +/- 0.03 detection
Forced photometry filter REJECTED candidate at 19:37:54.84 +23:46:57.5: ref_mag=13.00 +/- 0.02 new_mean_mag=12.6403 delta=0.36 (need > 0.90)
Forced photometry reference-image weighted average: 13.20 +/- 0.02
Forced photometry reference-image weighted average: 12.45 +/- 0.01
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:41:43.73 +18:59:40.4: 13.31 +/- 0.04 detection
Forced photometry filter REJECTED candidate at 19:29:56.90 +18:21:41.8: ref_mag=13.20 +/- 0.02 new_mean_mag=12.9606 delta=0.24 (need > 0.90)
Forced photometry reference-image weighted average: 13.13 +/- 0.02
Forced photometry filter REJECTED candidate at 19:17:53.38 +22:36:07.9: ref_mag=12.45 +/- 0.01 new_mean_mag=12.6917 delta=-0.24 (need > 0.90)
Forced photometry reference-image weighted average: 13.36 +/- 0.03
Forced photometry filter REJECTED candidate at 19:35:48.34 +17:49:57.4: ref_mag=13.36 +/- 0.03 new_mean_mag=13.1090 delta=0.25 (need > 0.90)
Forced photometry filter REJECTED candidate at 19:11:49.32 +20:10:48.5: ref_mag=13.13 +/- 0.02 new_mean_mag=13.0158 delta=0.12 (need > 0.90)
Forced photometry reference-image weighted average: 13.29 +/- 0.03
Forced photometry filter REJECTED candidate at 19:41:43.73 +18:59:40.4: ref_mag=13.29 +/- 0.03 new_mean_mag=12.7718 delta=0.52 (need > 0.90)
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:01:42.64 +20:46:56.7: 13.01 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.02
Forced photometry filter REJECTED candidate at 19:01:42.64 +20:46:56.7: ref_mag=12.97 +/- 0.02 new_mean_mag=12.9658 delta=0.00 (need > 0.90)
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 18:54:19.05 +24:53:11.0: 13.78 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.76 +/- 0.04
Forced photometry filter REJECTED candidate at 18:54:19.05 +24:53:11.0: ref_mag=13.76 +/- 0.04 new_mean_mag=13.0454 delta=0.72 (need > 0.90)
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:08:38.97 +19:23:52.4: 11.98 +/- 0.01 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:08:22.46 +21:34:02.0: 12.40 +/- 0.01 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:00:39.38 +21:01:48.8: 12.46 +/- 0.02 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:04:15.69 +21:13:04.2: 12.90 +/- 0.03 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:01:42.74 +22:52:29.3: 12.79 +/- 0.02 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:36:17.23 +21:57:18.2: 13.15 +/- 0.04 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:08:38.97 +19:23:52.4: 12.02 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.00 +/- 0.01
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 18:58:45.38 +25:27:20.4: 12.61 +/- 0.02 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:04:15.69 +21:13:04.2: 12.92 +/- 0.03 detection
Forced photometry filter REJECTED candidate at 19:08:38.97 +19:23:52.4: ref_mag=12.00 +/- 0.01 new_mean_mag=12.1602 delta=-0.16 (need > 0.90)
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:08:22.46 +21:34:02.0: 12.39 +/- 0.02 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:01:42.74 +22:52:29.3: 12.81 +/- 0.02 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:36:17.23 +21:57:18.2: 13.18 +/- 0.05 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:00:39.38 +21:01:48.8: 12.45 +/- 0.02 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:04:14.31 +21:12:39.9: 13.17 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.02
Forced photometry reference-image weighted average: 12.40 +/- 0.01
Forced photometry filter REJECTED candidate at 19:04:15.69 +21:13:04.2: ref_mag=12.91 +/- 0.02 new_mean_mag=12.4905 delta=0.42 (need > 0.90)
Forced photometry reference-image weighted average: 13.16 +/- 0.03
Forced photometry filter REJECTED candidate at 19:08:22.46 +21:34:02.0: ref_mag=12.40 +/- 0.01 new_mean_mag=12.1602 delta=0.24 (need > 0.90)
Forced photometry reference-image weighted average: 12.46 +/- 0.01
Forced photometry reference-image weighted average: 12.80 +/- 0.02
Forced photometry filter REJECTED candidate at 19:36:17.23 +21:57:18.2: ref_mag=13.16 +/- 0.03 new_mean_mag=12.6390 delta=0.53 (need > 0.90)
Forced photometry filter REJECTED candidate at 19:00:39.38 +21:01:48.8: ref_mag=12.46 +/- 0.01 new_mean_mag=12.3189 delta=0.14 (need > 0.90)
Forced photometry filter REJECTED candidate at 19:01:42.74 +22:52:29.3: ref_mag=12.80 +/- 0.02 new_mean_mag=12.4047 delta=0.39 (need > 0.90)
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 18:58:45.38 +25:27:20.4: 12.63 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.02
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:04:14.31 +21:12:39.9: 13.26 +/- 0.04 detection
Forced photometry filter REJECTED candidate at 18:58:45.38 +25:27:20.4: ref_mag=12.62 +/- 0.02 new_mean_mag=12.2899 delta=0.33 (need > 0.90)
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Forced photometry filter REJECTED candidate at 19:04:14.31 +21:12:39.9: ref_mag=13.21 +/- 0.02 new_mean_mag=12.8100 delta=0.40 (need > 0.90)
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:11:18.99 +22:55:15.9: 12.75 +/- 0.02 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:41:57.03 +18:35:09.7: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:22:35.63 +24:56:53.7: 12.69 +/- 0.03 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:22:35.63 +24:56:53.7: 12.75 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.72 +/- 0.02
Forced photometry filter REJECTED candidate at 19:22:35.63 +24:56:53.7: ref_mag=12.72 +/- 0.02 new_mean_mag=12.8377 delta=-0.12 (need > 0.90)
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:41:57.03 +18:35:09.7: 99.00 +/- 99.00 bad_region
Forced photometry filter REJECTED candidate at 19:41:57.03 +18:35:09.7: the position falls in a bad CCD region (bad_region.lst) on all measured reference images -- cannot perform the forced-photometry cross-check
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:11:18.99 +22:55:15.9: 12.75 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.75 +/- 0.01
Forced photometry filter REJECTED candidate at 19:11:18.99 +22:55:15.9: ref_mag=12.75 +/- 0.01 new_mean_mag=12.4977 delta=0.25 (need > 0.90)
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 18:56:20.39 +23:05:22.0: 13.47 +/- 0.04 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 18:56:20.39 +23:05:22.0: 13.56 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.03
Forced photometry filter REJECTED candidate at 18:56:20.39 +23:05:22.0: ref_mag=13.51 +/- 0.03 new_mean_mag=13.0172 delta=0.49 (need > 0.90)
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:14:22.62 +20:56:31.8: 13.63 +/- 0.05 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:41:34.76 +25:19:21.9: 13.79 +/- 0.05 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:37:10.14 +18:11:20.2: 13.15 +/- 0.03 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:14:22.62 +20:56:31.8: 13.70 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.66 +/- 0.04
Forced photometry filter REJECTED candidate at 19:14:22.62 +20:56:31.8: ref_mag=13.66 +/- 0.04 new_mean_mag=13.4356 delta=0.22 (need > 0.90)
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:41:34.76 +25:19:21.9: 13.83 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.04
Forced photometry filter KEPT candidate at 19:41:34.76 +25:19:21.9: ref_mag=13.81 +/- 0.04 new_mean_mag=12.6929 delta=1.12 (need > 0.90)
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:38:48.59 +20:48:32.7: 12.59 +/- 0.02 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:37:10.14 +18:11:20.2: 13.17 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.02
Forced photometry filter KEPT candidate at 19:37:10.14 +18:11:20.2: ref_mag=13.16 +/- 0.02 new_mean_mag=12.2029 delta=0.96 (need > 0.90)
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:38:48.59 +20:48:32.7: 12.59 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.59 +/- 0.01
Forced photometry filter KEPT candidate at 19:38:48.59 +20:48:32.7: ref_mag=12.59 +/- 0.01 new_mean_mag=11.6794 delta=0.91 (need > 0.90)
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:41:26.52 +24:54:55.2: 13.30 +/- 0.03 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:42:23.64 +25:17:59.3: 13.70 +/- 0.05 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:41:26.52 +24:54:55.2: 13.32 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.02
Forced photometry filter KEPT candidate at 19:41:26.52 +24:54:55.2: ref_mag=13.31 +/- 0.02 new_mean_mag=12.3395 delta=0.97 (need > 0.90)
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:42:23.64 +25:17:59.3: 13.66 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.03
Forced photometry filter KEPT candidate at 19:42:23.64 +25:17:59.3: ref_mag=13.68 +/- 0.03 new_mean_mag=12.6503 delta=1.03 (need > 0.90)
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:41:47.29 +19:51:26.0: 13.09 +/- 0.03 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:38:14.25 +21:15:17.1: 13.51 +/- 0.04 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:41:47.29 +19:51:26.0: 13.02 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.02
Forced photometry filter REJECTED candidate at 19:41:47.29 +19:51:26.0: ref_mag=13.05 +/- 0.02 new_mean_mag=12.6165 delta=0.44 (need > 0.90)
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:38:14.25 +21:15:17.1: 13.60 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.03
Forced photometry filter KEPT candidate at 19:38:14.25 +21:15:17.1: ref_mag=13.55 +/- 0.03 new_mean_mag=12.6322 delta=0.92 (need > 0.90)
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:37:41.06 +18:16:58.6: 13.78 +/- 0.06 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:37:41.06 +18:16:58.6: 13.95 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.85 +/- 0.05
Forced photometry filter KEPT candidate at 19:37:41.06 +18:16:58.6: ref_mag=13.85 +/- 0.05 new_mean_mag=12.4720 delta=1.38 (need > 0.90)
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:36:57.34 +24:15:05.0: 13.04 +/- 0.03 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:38:31.88 +20:59:27.0: 14.27 +/- 0.07 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:36:57.34 +24:15:05.0: 13.10 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.02
Forced photometry filter KEPT candidate at 19:36:57.34 +24:15:05.0: ref_mag=13.07 +/- 0.02 new_mean_mag=12.1281 delta=0.94 (need > 0.90)
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:38:31.88 +20:59:27.0: 14.17 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.22 +/- 0.05
Forced photometry filter KEPT candidate at 19:38:31.88 +20:59:27.0: ref_mag=14.22 +/- 0.05 new_mean_mag=13.1093 delta=1.11 (need > 0.90)
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:40:57.01 +25:16:36.9: 14.07 +/- 0.06 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:40:57.01 +25:16:36.9: 14.11 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.09 +/- 0.05
Forced photometry filter KEPT candidate at 19:40:57.01 +25:16:36.9: ref_mag=14.09 +/- 0.05 new_mean_mag=12.9357 delta=1.15 (need > 0.90)
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:42:24.18 +22:09:43.6: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:42:24.18 +22:09:43.6: 99.00 +/- 99.00 bad_region
Forced photometry filter REJECTED candidate at 19:42:24.18 +22:09:43.6: the position falls in a bad CCD region (bad_region.lst) on all measured reference images -- cannot perform the forced-photometry cross-check
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:37:48.94 +24:33:06.9: 12.81 +/- 0.03 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:35:05.65 +19:23:07.6: 13.96 +/- 0.06 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:37:48.94 +24:33:06.9: 12.87 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.02
Forced photometry filter REJECTED candidate at 19:37:48.94 +24:33:06.9: ref_mag=12.84 +/- 0.02 new_mean_mag=12.0598 delta=0.78 (need > 0.90)
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:39:36.46 +25:05:22.4: 13.93 +/- 0.07 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:40:37.60 +25:48:06.4: 13.61 +/- 0.05 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:35:05.65 +19:23:07.6: 14.05 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.00 +/- 0.04
Forced photometry filter KEPT candidate at 19:35:05.65 +19:23:07.6: ref_mag=14.00 +/- 0.04 new_mean_mag=13.0128 delta=0.99 (need > 0.90)
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:39:36.46 +25:05:22.4: 13.87 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.90 +/- 0.05
Forced photometry filter KEPT candidate at 19:39:36.46 +25:05:22.4: ref_mag=13.90 +/- 0.05 new_mean_mag=12.8240 delta=1.08 (need > 0.90)
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:40:37.60 +25:48:06.4: 13.47 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.53 +/- 0.03
Forced photometry filter KEPT candidate at 19:40:37.60 +25:48:06.4: ref_mag=13.53 +/- 0.03 new_mean_mag=12.5517 delta=0.98 (need > 0.90)
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:39:30.68 +24:11:42.3: 13.84 +/- 0.06 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:41:49.55 +26:10:35.6: 12.99 +/- 0.03 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:41:34.34 +25:11:40.8: 13.39 +/- 0.04 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:39:30.68 +24:11:42.3: 13.89 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.86 +/- 0.04
Forced photometry filter KEPT candidate at 19:39:30.68 +24:11:42.3: ref_mag=13.86 +/- 0.04 new_mean_mag=12.8562 delta=1.01 (need > 0.90)
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:41:49.55 +26:10:35.6: 12.93 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.02
Forced photometry filter KEPT candidate at 19:41:49.55 +26:10:35.6: ref_mag=12.96 +/- 0.02 new_mean_mag=11.9710 delta=0.99 (need > 0.90)
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:37:29.72 +23:30:37.9: 14.71 +/- 0.13 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:38:56.89 +24:13:03.4: 13.57 +/- 0.04 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:41:34.34 +25:11:40.8: 13.34 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.03
Forced photometry filter KEPT candidate at 19:41:34.34 +25:11:40.8: ref_mag=13.37 +/- 0.03 new_mean_mag=12.4033 delta=0.96 (need > 0.90)
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:38:56.89 +24:13:03.4: 13.59 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.58 +/- 0.03
Forced photometry filter KEPT candidate at 19:38:56.89 +24:13:03.4: ref_mag=13.58 +/- 0.03 new_mean_mag=12.6523 delta=0.93 (need > 0.90)
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:37:29.72 +23:30:37.9: 14.65 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.68 +/- 0.09
Forced photometry filter KEPT candidate at 19:37:29.72 +23:30:37.9: ref_mag=14.68 +/- 0.09 new_mean_mag=12.9954 delta=1.69 (need > 0.90)
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:41:54.35 +25:38:48.8: 13.74 +/- 0.05 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:41:54.35 +25:38:48.8: 13.62 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.03
Forced photometry filter KEPT candidate at 19:41:54.35 +25:38:48.8: ref_mag=13.67 +/- 0.03 new_mean_mag=12.6812 delta=0.99 (need > 0.90)
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 18:55:20.32 +25:41:34.4: 13.97 +/- 0.08 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:40:30.46 +18:55:05.4: 13.62 +/- 0.06 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 18:55:20.32 +25:41:34.4: 13.84 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.90 +/- 0.05
Forced photometry filter KEPT candidate at 18:55:20.32 +25:41:34.4: ref_mag=13.90 +/- 0.05 new_mean_mag=12.8003 delta=1.10 (need > 0.90)
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:37:10.54 +18:20:09.9: 13.84 +/- 0.06 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:39:40.24 +23:47:34.9: 13.79 +/- 0.06 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:40:30.46 +18:55:05.4: 13.64 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.63 +/- 0.04
Forced photometry filter REJECTED candidate at 19:40:30.46 +18:55:05.4: ref_mag=13.63 +/- 0.04 new_mean_mag=12.8637 delta=0.77 (need > 0.90)
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:37:10.54 +18:20:09.9: 13.79 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.82 +/- 0.04
Forced photometry filter KEPT candidate at 19:37:10.54 +18:20:09.9: ref_mag=13.82 +/- 0.04 new_mean_mag=12.8290 delta=0.99 (need > 0.90)
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:39:40.24 +23:47:34.9: 13.73 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.76 +/- 0.04
Forced photometry filter KEPT candidate at 19:39:40.24 +23:47:34.9: ref_mag=13.76 +/- 0.04 new_mean_mag=12.7163 delta=1.05 (need > 0.90)
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:38:41.68 +18:20:16.3: 13.59 +/- 0.05 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:42:10.71 +25:14:36.2: 13.53 +/- 0.04 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:38:41.68 +18:20:16.3: 13.50 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.54 +/- 0.03
Forced photometry filter KEPT candidate at 19:38:41.68 +18:20:16.3: ref_mag=13.54 +/- 0.03 new_mean_mag=12.4129 delta=1.13 (need > 0.90)
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:42:10.71 +25:14:36.2: 13.61 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.03
Forced photometry filter KEPT candidate at 19:42:10.71 +25:14:36.2: ref_mag=13.56 +/- 0.03 new_mean_mag=12.6186 delta=0.95 (need > 0.90)
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-24-54_20.00sec_-0.00C_LIGHT_1311.fits at 19:38:57.41 +23:32:12.4: 13.83 +/- 0.07 detection
Forced photometry on wcs_Vul-01-Q2b1x1_2026-05-17_05-25-50_20.00sec_-0.00C_LIGHT_1312.fits at 19:38:57.41 +23:32:12.4: 13.85 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.84 +/- 0.05
Forced photometry filter KEPT candidate at 19:38:57.41 +23:32:12.4: ref_mag=13.84 +/- 0.05 new_mean_mag=12.4475 delta=1.39 (need > 0.90)
Adding exclusion_list_local.txt__out141431.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out157742.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out158201.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159254.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175679.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out179325.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out185924.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out94797.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 34s
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: 13s
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Considering the candidate 261390_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 261390_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
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Considering the candidate 261394_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 261394_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
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Considering the candidate 261405_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 261405_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
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Considering the candidate 261409_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 261409_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
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Considering the candidate 261411_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 261411_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
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Considering the candidate 261417_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 261417_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
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Considering the candidate 261418_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 261418_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
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Considering the candidate 261420_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 261420_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
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Considering the candidate 261430_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 261430_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
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Considering the candidate 261475_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 261475_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 19:41:53.22 +18:01:34.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261558_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 261558_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 19:28:53.31 +24:38:47.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261621_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 261621_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 19:41:53.66 +18:07:41.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261670_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 261670_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 19:41:56.88 +18:33:39.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261742_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 261742_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
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Considering the candidate 261780_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 261780_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 19:07:57.55 +21:42:40.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 261820_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 261820_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
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Considering the candidate 261823_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 261823_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
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Considering the candidate 261846_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 261846_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
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Considering the candidate 261888_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 261888_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
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Considering the candidate 261906_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 261906_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
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Considering the candidate 261924_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 261924_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 19:01:01.18 +19:17:47.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 261929_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 261929_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 19:37:50.14 +22:48:55.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261984_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 261984_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
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Considering the candidate 262046_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 262046_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
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Considering the candidate 262051_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 262051_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 18:54:29.02 +20:20:17.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262062_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 262062_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 19:37:55.78 +18:36:44.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262071_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 262071_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 19:22:55.63 +26:14:40.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 262088_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 262088_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
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Considering the candidate 262095_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 262095_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
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Considering the candidate 262150_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 262150_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 19:35:56.72 +23:52:19.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262153_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 262153_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 19:01:23.36 +20:44:47.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262161_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 262161_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
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Considering the candidate 262178_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 262178_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 19:07:57.10 +19:52:00.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262188_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 262188_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 19:36:57.18 +23:32:18.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262198_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 262198_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 19:06:19.99 +21:22:36.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262208_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 262208_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 19:12:28.73 +23:28:43.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262264_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 262264_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
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Considering the candidate 262276_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 262276_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 19:36:03.45 +20:02:42.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262286_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 262286_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 19:06:20.14 +20:40:15.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262337_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 262337_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 19:12:37.34 +21:31:45.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 262362_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 262362_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 19:04:34.27 +22:06:46.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262369_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 262369_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 18:57:57.29 +20:20:45.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262389_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 262389_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
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Considering the candidate 195933_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 195933_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 84727_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 84727_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 19:37:37.77 +20:45:06.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33827_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 33827_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 19:41:13.23 +18:23:10.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 29384_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 29384_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 86318_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 86318_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 57768_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 57768_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 19:37:20.88 +19:28:56.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21043_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 21043_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 19:40:32.97 +17:46:00.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 95820_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 95820_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 19:39:35.87 +21:17:33.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 157328_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 157328_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 19:41:30.69 +24:07:42.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 59719_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 59719_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 19:41:24.44 +19:34:47.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 74524_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 74524_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 19:37:36.53 +20:15:55.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105368_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 105368_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 19:38:17.56 +21:47:24.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 175679_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 175679_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 196935_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 196935_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 244292_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 244292_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 19:14:57.05 +22:04:29.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 244144_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 244144_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 19:40:11.87 +18:47:29.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 244143_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 244143_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 19:40:44.42 +19:01:24.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 83667_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 83667_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 19:40:45.84 +20:41:35.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 66065_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 66065_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
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Considering the candidate 94797_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 94797_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51941_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 51941_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 19:41:42.96 +19:12:52.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 142770_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 142770_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 19:39:12.27 +23:32:44.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31280_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 31280_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159254_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 159254_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 89264_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 89264_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197594_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 197594_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 152909_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 152909_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 19:40:34.50 +23:58:10.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251635_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 251635_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 122847_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 122847_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 18:56:03.86 +22:31:30.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 166176_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 166176_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250979_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 250979_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 19:06:19.84 +21:32:19.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 83948_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 83948_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 19:39:51.46 +20:41:08.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54938_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 54938_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 185924_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 185924_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 179325_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 179325_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 46105_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 46105_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 19:33:22.31 +18:58:39.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 44155_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 44155_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 19:36:16.70 +18:52:45.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 156424_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 156424_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 18:56:59.68 +24:01:26.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 157742_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 157742_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 225681_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 225681_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199324_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 199324_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 141431_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 141431_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 158201_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 158201_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52717_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 52717_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 19:40:22.51 +19:15:54.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 162890_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 162890_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
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Considering the candidate 170824_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 170824_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 19:37:02.41 +24:45:08.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 188229_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 188229_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 229837_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 229837_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 18:55:10.16 +25:52:56.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54749_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 54749_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 19:37:35.88 +19:22:10.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 97781_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 97781_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 19:41:47.63 +21:23:44.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 184385_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 184385_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62266_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 62266_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 19:41:06.83 +19:41:53.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 45147_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 45147_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32313_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 32313_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 148677_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 148677_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39354_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 39354_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 19:32:51.82 +18:40:18.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 74819_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 74819_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 19:41:13.88 +20:15:48.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32652_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 32652_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198244_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 198244_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 244853_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 244853_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 19:42:01.53 +19:10:46.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 142860_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 142860_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 244770_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071
The candidate 244770_fd_Vul-01-Q2b1x1_2026-06-07_22-47-53_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 19:41:21.91 +18:05:06.1 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 2s
make_report_in_HTML.sh TOTAL: 49s
Prepared the HTML report for the field Vul-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
19:37:29.72 +23:30:37.9
19:38:57.41 +23:32:12.4
19:39:40.24 +23:47:34.9
19:39:30.68 +24:11:42.3
19:38:56.89 +24:13:03.4
19:36:57.34 +24:15:05.0
19:41:26.52 +24:54:55.2
19:39:36.46 +25:05:22.4
18:55:20.32 +25:41:34.4
19:40:37.60 +25:48:06.4
19:41:54.35 +25:38:48.8
19:41:34.76 +25:19:21.9
19:42:23.64 +25:17:59.3
19:40:57.01 +25:16:36.9
19:42:10.71 +25:14:36.2
19:41:34.34 +25:11:40.8
19:41:49.55 +26:10:35.6
19:37:10.14 +18:11:20.2
19:37:41.06 +18:16:58.6
19:37:10.54 +18:20:09.9
19:38:41.68 +18:20:16.3
19:35:05.65 +19:23:07.6
19:38:48.59 +20:48:32.7
19:38:31.88 +20:59:27.0
19:38:14.25 +21:15:17.1
########### Completed Vul-01-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
19:41:34.76 +25:19:21.9
19:37:10.14 +18:11:20.2
19:38:48.59 +20:48:32.7
19:41:26.52 +24:54:55.2
19:42:23.64 +25:17:59.3
19:38:14.25 +21:15:17.1
19:37:41.06 +18:16:58.6
19:36:57.34 +24:15:05.0
19:38:31.88 +20:59:27.0
19:40:57.01 +25:16:36.9
19:35:05.65 +19:23:07.6
19:40:37.60 +25:48:06.4
19:39:36.46 +25:05:22.4
19:39:30.68 +24:11:42.3
19:41:49.55 +26:10:35.6
19:41:34.34 +25:11:40.8
19:37:29.72 +23:30:37.9
19:38:56.89 +24:13:03.4
19:41:54.35 +25:38:48.8
18:55:20.32 +25:41:34.4
19:37:10.54 +18:20:09.9
19:39:40.24 +23:47:34.9
19:38:41.68 +18:20:16.3
19:42:10.71 +25:14:36.2
19:38:57.41 +23:32:12.4
###################################################################################
19:41:34.76 +25:19:21.9 -- not an asteroid (will add it to exclusion list)
19:37:10.14 +18:11:20.2 -- not an asteroid (will add it to exclusion list)
19:38:48.59 +20:48:32.7 -- not an asteroid (will add it to exclusion list)
19:41:26.52 +24:54:55.2 -- not an asteroid (will add it to exclusion list)
19:42:23.64 +25:17:59.3 -- not an asteroid (will add it to exclusion list)
19:38:14.25 +21:15:17.1 -- not an asteroid (will add it to exclusion list)
19:37:41.06 +18:16:58.6 -- not an asteroid (will add it to exclusion list)
19:36:57.34 +24:15:05.0 -- not an asteroid (will add it to exclusion list)
19:38:31.88 +20:59:27.0 -- not an asteroid (will add it to exclusion list)
19:40:57.01 +25:16:36.9 -- not an asteroid (will add it to exclusion list)
19:35:05.65 +19:23:07.6 -- not an asteroid (will add it to exclusion list)
19:40:37.60 +25:48:06.4 -- not an asteroid (will add it to exclusion list)
19:39:36.46 +25:05:22.4 -- not an asteroid (will add it to exclusion list)
19:39:30.68 +24:11:42.3 -- not an asteroid (will add it to exclusion list)
19:41:49.55 +26:10:35.6 -- not an asteroid (will add it to exclusion list)
19:41:34.34 +25:11:40.8 -- not an asteroid (will add it to exclusion list)
19:37:29.72 +23:30:37.9 -- not an asteroid (will add it to exclusion list)
19:38:56.89 +24:13:03.4 -- not an asteroid (will add it to exclusion list)
19:41:54.35 +25:38:48.8 -- not an asteroid (will add it to exclusion list)
18:55:20.32 +25:41:34.4 -- not an asteroid (will add it to exclusion list)
19:37:10.54 +18:20:09.9 -- not an asteroid (will add it to exclusion list)
19:39:40.24 +23:47:34.9 -- not an asteroid (will add it to exclusion list)
19:38:41.68 +18:20:16.3 -- not an asteroid (will add it to exclusion list)
19:42:10.71 +25:14:36.2 -- not an asteroid (will add it to exclusion list)
19:38:57.41 +23:32:12.4 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
18:55:20.32 +25:41:34.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:35:05.65 +19:23:07.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:36:57.34 +24:15:05.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:37:10.14 +18:11:20.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:37:10.54 +18:20:09.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:37:29.72 +23:30:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:37:41.06 +18:16:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:38:14.25 +21:15:17.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:38:31.88 +20:59:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:38:41.68 +18:20:16.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:38:48.59 +20:48:32.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:38:56.89 +24:13:03.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:38:57.41 +23:32:12.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:39:30.68 +24:11:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:39:36.46 +25:05:22.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:39:40.24 +23:47:34.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:40:37.60 +25:48:06.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:40:57.01 +25:16:36.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:41:26.52 +24:54:55.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:41:34.34 +25:11:40.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:41:34.76 +25:19:21.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:41:49.55 +26:10:35.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:41:54.35 +25:38:48.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:42:10.71 +25:14:36.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:42:23.64 +25:17:59.3 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
18:55:20.32 +25:41:34.4 -- a known variable star
19:35:05.65 +19:23:07.6 -- a known variable star
19:36:57.34 +24:15:05.0 -- a known variable star
19:37:10.14 +18:11:20.2 -- a known variable star
19:37:10.54 +18:20:09.9 -- a known variable star
19:37:29.72 +23:30:37.9 -- a known variable star
19:37:41.06 +18:16:58.6 -- a known variable star
19:38:14.25 +21:15:17.1 -- a known variable star
19:38:31.88 +20:59:27.0 -- a known variable star
19:38:41.68 +18:20:16.3 -- a known variable star
19:38:48.59 +20:48:32.7 -- a known variable star
19:38:56.89 +24:13:03.4 -- not a known variable star
19:38:57.41 +23:32:12.4 -- a known variable star
19:39:30.68 +24:11:42.3 -- a known variable star
19:39:36.46 +25:05:22.4 -- a known variable star
19:39:40.24 +23:47:34.9 -- a known variable star
19:40:37.60 +25:48:06.4 -- a known variable star
19:40:57.01 +25:16:36.9 -- not a known variable star
19:41:26.52 +24:54:55.2 -- a known variable star
19:41:34.34 +25:11:40.8 -- a known variable star
19:41:34.76 +25:19:21.9 -- a known variable star
19:41:49.55 +26:10:35.6 -- a known variable star
19:41:54.35 +25:38:48.8 -- not a known variable star
19:42:10.71 +25:14:36.2 -- not a known variable star
19:42:23.64 +25:17:59.3 -- a known variable star
Found 4 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
25 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
###################################################################################
exclusion_list_gaiadr2.txt NOT FOUND
exclusion_list_apass.txt NOT FOUND
IS_THIS_TEST_RUN= NO ALLOW_EXCLUSION_LIST_UPDATE= YES
#### Adding the following to the exclusion list ####
18:55:20.32 +25:41:34.4
19:35:05.65 +19:23:07.6
19:36:57.34 +24:15:05.0
19:37:10.14 +18:11:20.2
19:37:10.54 +18:20:09.9
19:37:29.72 +23:30:37.9
19:37:41.06 +18:16:58.6
19:38:14.25 +21:15:17.1
19:38:31.88 +20:59:27.0
19:38:41.68 +18:20:16.3
19:38:48.59 +20:48:32.7
19:38:56.89 +24:13:03.4
19:38:57.41 +23:32:12.4
19:39:30.68 +24:11:42.3
19:39:36.46 +25:05:22.4
19:39:40.24 +23:47:34.9
19:40:37.60 +25:48:06.4
19:40:57.01 +25:16:36.9
19:41:26.52 +24:54:55.2
19:41:34.34 +25:11:40.8
19:41:34.76 +25:19:21.9
19:41:49.55 +26:10:35.6
19:41:54.35 +25:38:48.8
19:42:10.71 +25:14:36.2
19:42:23.64 +25:17:59.3
####################################################
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461199.65770866 -observatory V36
06:43:31.79 +25:00:27.6 Mercury (0.1mag)
07:42:40.87 +23:23:10.4 Venus (-4.0mag)
02:49:30.56 +15:42:22.8 Mars (1.3mag)
07:48:24.54 +21:31:31.5 Jupiter (-1.9mag)
00:49:21.86 +02:48:37.7 Saturn (0.9mag)
04:00:11.92 +20:25:26.4 Uranus (5.8mag)
00:16:08.41 +00:16:47.7 Neptune (7.8mag)
20:33:21.51 -23:04:32.0 Pluto (14.5mag)
23:01:23.39 -05:50:59.9 Moon (-10.4mag)
-rw-r--r-- 1 apache apache 362 Jun 8 00:14 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461199.65770866:
07:48:24.79 +21:31:32.9 Io (6.0mag)
07:48:24.24 +21:31:34.6 Europa (6.2mag)
07:48:08.66 +21:32:18.7 Ganymede (5.6mag)
07:48:43.43 +21:30:30.6 Callisto (6.7mag)
07:48:42.02 +21:07:49.0 Himalia (15.6mag)
07:48:28.98 +21:31:17.9 Thebe (16.5mag)
07:48:41.51 +21:23:16.4 Elara (17.5mag)
07:50:35.12 +21:43:14.5 Pasiphae (17.7mag)
07:54:59.71 +21:33:13.8 Carme (18.9mag)
00:49:12.37 +02:48:36.8 Titan (8.7mag)
00:49:18.91 +02:48:51.0 Rhea (9.9mag)
00:49:54.15 +02:50:46.9 Iapetus (11.3mag)
00:49:17.72 +02:48:14.8 Hyperion (14.7mag)
00:50:04.16 +02:50:34.5 Phoebe (16.7mag)
-rw-r--r-- 1 apache apache 568 Jun 8 00:14 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461199.65770866:
17:26:46.53 -35:14:19.9 JWST
14:24:52.25 +57:41:14.5 Chandra
18:28:16.55 -27:07:40.7 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jun 8 00:14 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461199.65770866 -observatory V36
18:43:32.19 -32:39:04.7 13.6mag P/2010 H2 (Vales)
05:53:26.08 -68:03:52.0 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:49:02.74 +31:58:03.2 17.5mag C/2017 K2 (PANSTARRS)
17:14:44.84 +15:21:00.4 17.8mag C/2021 G2 (ATLAS)
21:11:56.61 -49:30:21.7 16.9mag P/2021 N1 (ZTF)
23:12:38.50 +31:35:26.3 17.2mag C/2022 E2 (ATLAS)
05:33:59.82 +26:58:31.1 16.5mag C/2022 N2 (PANSTARRS)
09:29:42.08 +31:05:02.3 16.6mag C/2022 QE78 (ATLAS)
08:50:31.57 +03:55:48.7 17.7mag C/2022 R6 (PANSTARRS)
18:28:14.79 +21:36:06.0 17.8mag C/2023 A3 (Tsuchinshan-ATLAS)
15:19:23.20 -11:00:30.9 17.6mag P/2023 B1 (PANSTARRS)
22:14:26.65 +66:31:34.8 17.7mag C/2023 H5 (Lemmon)
17:46:28.72 -06:41:08.3 13.7mag C/2023 R1 (PANSTARRS)
13:18:07.02 +83:00:06.4 17.9mag C/2023 X2 (Lemmon)
07:10:21.79 +64:18:28.4 17.7mag C/2024 A1 (ATLAS)
06:47:12.90 +27:49:51.8 13.6mag C/2024 E1 (Wierzchos)
15:37:19.09 +13:31:23.5 17.4mag C/2024 G6 (ATLAS)
20:13:04.23 +31:07:27.8 14.0mag C/2024 J3 (ATLAS)
04:17:59.33 -15:57:15.4 16.0mag C/2024 T5 (ATLAS)
06:05:52.60 +34:29:52.7 17.9mag C/2025 J1 (Borisov)
11:34:55.43 +52:45:04.7 17.4mag C/2025 L1 (ATLAS)
06:44:53.83 -10:52:05.3 14.1mag C/2025 R3 (PANSTARRS)
09:24:07.89 +23:20:25.9 17.9mag C/2025 V2 (Rankin)
12:39:42.15 +04:41:28.3 17.2mag C/2025 Y1 (ATLAS)
18:12:56.77 +75:07:27.6 17.9mag C/2026 A2 (Bok)
02:00:36.03 +43:24:45.6 16.1mag C/2026 B2 (Sun-Gao)
11:11:18.30 -03:44:46.8 16.5mag A/2026 E1
20:23:35.01 -08:34:00.7 8.7mag 10P/Tempel
11:01:59.80 -00:58:02.9 16.0mag 29P/Schwassmann-Wachmann
03:11:39.79 +25:38:26.8 17.7mag 47P/Ashbrook-Jackson
08:59:54.07 +23:46:47.1 16.9mag 63P/Wild
00:26:53.71 -06:22:11.5 15.7mag 65P/Gunn
06:43:19.20 +33:25:34.9 16.9mag 76P/West-Kohoutek-Ikemura
03:09:05.48 +17:12:43.1 13.8mag 78P/Gehrels
01:20:40.68 +04:50:28.7 15.6mag 88P/Howell
04:54:31.25 +30:18:01.1 15.2mag 93P/Lovas
02:42:50.72 +27:37:12.6 17.6mag 114P/Wiseman-Skiff
06:50:27.55 +33:02:22.6 15.6mag 123P/West-Hartley
09:50:06.89 +14:39:12.1 16.5mag 124P/Mrkos
03:58:58.44 +19:14:52.9 16.4mag 128P/Shoemaker-Holt
04:33:29.37 +19:04:58.2 17.7mag 131P/Mueller
05:58:09.12 +18:40:10.8 14.6mag 141P/Machholz
06:00:47.26 +17:40:24.2 14.6mag 141P-A/Machholz
04:53:54.20 +16:10:07.2 11.6mag 141P-D/Machholz
02:57:39.09 -24:42:17.0 16.8mag 161P/Hartley-IRAS
03:41:25.49 +23:47:41.3 14.9mag 162P/SidingSpring
19:36:38.31 +01:43:06.3 16.9mag 169P/NEAT
00:18:14.14 +02:27:29.3 17.9mag 220P/McNaught
16:52:12.74 -08:28:39.4 16.4mag 235P/LINEAR
07:34:34.39 +35:29:36.7 17.5mag 240P/NEAT
00:32:15.17 -02:29:05.2 16.4mag 260P/McNaught
04:04:07.41 +32:28:27.6 17.6mag 295P/LINEAR
23:52:00.75 -09:45:27.3 17.6mag 320P/McNaught
15:15:15.32 +08:06:03.9 17.4mag 391P/Kowalski
08:07:06.44 +20:44:54.1 17.9mag 450P/LONEOS
06:59:54.72 +41:41:57.1 17.8mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.7K Jun 8 00:14 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
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
11:44:32.95 -68:48:30.00 ASASSN-26no 2026-05-24 8.41
19:00:42.82 -48:31:01.60 ASASSN-26dp 2026-05-22.31 -3.28
14:23:56.59 -58:37:47.40 ASASSN-26dn 2026-05-20.01 14.59
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
16:21:48.82 -61:36:13.20 ASASSN-26dd 2026-05-5.21 15.15
14:26:40.22 -24:48:37.50 AT2026lig 2026-05-4.27 14.63
13:17:51.04 +30:25:13.50 SN2026kcp 2026-05-4.46 16.43
11:27:55.57 -13:38:56.90 SN2026kza 2026-05-1.08 15.59
22:28:27.10 +30:17:54.30 SN 2026fov 2026-04-29.6 14.36
21:00:10.71 -32:17:03.90 AT2026kis 2026-04-27.36 16.15
14:32:57.37 -58:13:26.40 ASASSN-26dc 2026-04-27.27 13.42
15:32:05.35 -43:54:34.60 ASASSN-26db 2026-04-27.37 16.06
16:34:34.97 -54:34:58.00 ASASSN-26da 2026-04-25.32 16.11
10:06:55.04 -01:13:49.70 SN2026jsg 2026-04-24.99 16.28
15:15:57.17 +56:18:32.80 SN2026kid 2026-04-24.52 -3.65
07:58:28.45 +57:03:42.40 AT2026kcf 2026-04-24.2 16.89
11:38:21.80 -50:43:06.50 SN2026jkb 2026-04-24.24 15.38
10:06:11.41 -39:41:04.20 AT2026dil 2026-04-24.2 16.85
14:21:40.08 +13:13:46.30 SN2026jlm 2026-04-22.16 15.12
10:53:55.52 -16:06:06.00 ASASSN-26cz 2026-04-22.28 16.29
20:07:38.15 -21:07:05.40 2026-05-25.18 -1.12
13:45:02.03 +15:17:14.50 ASASSN-26cy 2026-04-21.27 15.78
13:20:52.22 -35:57:03.60 AT2026jcm 2026-04-19.01 16.65
13:36:15.66 -36:53:48.40 SN 2026iqy 2026-04-18.92 17.31
06:34:01.33 -40:07:34.00 ASASSN-26cx 2026-04-19.07 16.16
23:33:57.97 -45:12:11.90 SN 2026idu 2026-04-19.41 15.9
12:10:50.92 +66:55:31.20 SN 2026icv 2026-04-17.14 16.03
21:36:59.06 -60:43:35.90 ASASSN-26cv 2026-04-17.35 -1.18
08:13:26.26 -27:07:30.50 ASASSN-26cw 2026-04-17.07 -1.01
14:49:14.13 -27:29:20.60 ASASSN-26cu 2026-04-16.06 14.03
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
20:07:38.15 -21:07:05.40 2026-05-25.18 -1.12
12:23:20.40 +04:53:39.10 AT2026ixd 2026-04-12.14 17.65
17:46:09.76 -61:19:50.40 SN2026icy 2026-04-12.2 17.03
09:25:46.42 +02:13:46.30 SN2026gud 2026-04-11.98 16.49
16:52:15.46 -60:27:45.90 ASASSN-26cs 2026-04-12.4 15.5
04:20:55.37 -51:15:31.10 ASASSN-26cr 2026-04-12.01 15.37
22:25:39.35 +36:45:06.90 AT2026ihl 2026-04-10.48 14.21
19:40:44.94 +00:41:03.80 AT2026imw 2026-04-10.32 16.06
19:52:04.70 +05:53:33.50 ASASSN-26cq 2026-04-9.31 14.98
16:08:18.39 -64:11:08.80 ASASSN-26cp 2026-04-9.29 13.32
09:22:22.90 -61:02:43.70 SN2026idh 2026-04-7.97 16.34
05:06:54.12 -19:42:26.40 AT2026imr 2026-04-8 17.49
07:14:55.34 -36:03:21.40 AT2026hei 2026-04-8.12 16.7
21:35:33.14 -19:01:34.80 AT2026ihm 2026-04-8.36 16.7
04:28:24.08 -32:25:35.30 AT2026imo 2026-04-8.02 16.81
05:10:35.79 -39:38:40.80 SN 2026hnn 2026-04-7.04 17.07
09:54:32.04 -01:17:25.80 ASASSN-26cn 2026-04-7.01 15.58
07:46:24.43 -77:29:35.90 ASASSN-26co 2026-04-7.15 14.93
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.70 -27:51:49.80 SN2026gvk 2026-03-30 15.48
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.80 -63:44:05.50 ASASSN-26ch 2026-03-27.86 13.02
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.88 -53:16:33.80 ASASSN-26cc 2026-03-20.04 15.48
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
-rw-r--r-- 1 apache apache 5.6K Jun 8 00:14 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
00:43:38.36 +41:15:32.4 PNV J00433836+4115324 2026-04-08.079 17.2mag
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
00:43:35.02 +41:46:28.0 PNV J00433502+4146280 2026-04-23.056 15.9mag
00:42:55.64 +41:14:12.2 PNV J00425564+4114122 2026-04-24.042 16.2mag
21:14:03.38 +56:46:44.1 TCP J21140338+5646441 2026-05-05.3534 16.7mag
15:03:05.19 +22:02:04.1 TCP J15030519+2202041 2026-05-08.3260 13.9mag
07:15:18.25 +47:53:16.7 TCP J07151825+4753167 2026-05-09.1599 14.4mag
16:00:18.44 -22:30:10.6 TCP J16001844-2230106 2026-05-09.6135 13.3mag
00:42:47.45 +41:16:58.5 PNV J00424745+4116585 2026-05-10.030 16.8mag
09:55:02.89 +69:02:13.8 PNV J09550289+6902138 2026-05-18.925 20.7mag
00:43:01.82 +41:18:16.6 PNV J00430182+4118166 2026-05-21.8651 18.83Cmag
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
-rw-r--r-- 1 apache apache 189K Jun 8 00:14 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
16:39:35.110 +15:17:58.28 AT 2026nsc 2026-05-09.80 20.76
16:42:48.680 +20:27:18.30 AT 2026nsb 2026-05-09.80 20.54
13:34:03.440 +31:37:31.73 AT 2026nsa 2026-05-07.80 21.26
13:50:28.150 +02:34:54.72 AT 2026nrz 2026-05-22.72 21.54
13:43:59.750 +03:47:21.63 AT 2026nry 2026-05-22.69 22.05
13:17:26.150 -01:26:00.12 AT 2026nrx 2026-05-21.64 21.7
00:35:20.216 -08:28:38.64 AT 2026nrw 2026-05-19.42 18.74
23:50:43.016 -01:09:12.25 AT 2026nrv 2026-05-23.48 19.5028
22:36:47.715 +37:31:34.81 AT 2026nru 2026-05-22.43 19.4626
23:58:04.247 +20:56:44.66 AT 2026nrt 2026-05-23.48 20.1237
16:08:58.229 +36:53:23.76 AT 2026nrs 2026-05-21.36 20.3819
19:44:04.734 +84:44:44.91 SN 2026nrr 2026-05-25.47 17.808
21:42:24.388 -20:21:08.51 SN 2026nrq 2026-05-25.56 18.623
22:03:20.669 -84:55:27.45 AT 2026nrp 2026-05-22.30 19.244
23:07:53.376 -39:04:26.84 AT 2026nro 2026-05-22.38 19.567
00:40:07.848 -39:10:21.32 AT 2026nrn 2026-05-12.41 18.737
23:05:28.381 -21:25:50.28 AT 2026nrm 2026-05-25.58 18.887
19:27:28.750 -48:42:52.35 AT 2026nrl 2026-05-22.24 19.107
12:33:38.422 +12:02:05.88 AT 2026nrk 2026-05-25.29 21.322
12:32:27.199 +02:39:54.51 AT 2026nrj 2026-05-25.29 21.0728
-rw-r--r-- 1 apache apache 30K Jun 8 00:14 tns_transients_list.txt
