This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Ser-07-Q2b1x1_041149_TTUQ2b1x1_928637_e4bqkijR
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 07 18.3826 2461239.8826 11.94 18:07:13.64 -05:07:28.9
23.26196 7.42384 galactic Ser Second-epoch detections are separated by 1.3" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J271.8062-05.1194 | 18:07:13.67 -05:07:29.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: M5 (LAMOST DR5) J-Ks=1.556+/-0.037 (Very red! L if it's a dwarf)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 18:07:13.64 -05:07:28.9: 12.92 +/- 0.03 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 18:07:13.64 -05:07:28.9: 12.88 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 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!
TCP 2026 07 18.3826* 18 07 13.64 -05 07 28.9 11.9 U Ser 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
ATO J271.8062-05.1194,2461239.8826,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J271.8062-05.1194 20260718.3826 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.3826 2461239.8826 11.60 17:51:01.41 -05:18:50.4
21.13759 10.87534 galactic Oph Second-epoch detections are separated by 1.6" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4175310297408867328 | 17:51:01.35 -05:18:50.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.398+/-0.031 (Very red! L if it's a dwarf)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 17:51:01.41 -05:18:50.4: 12.77 +/- 0.02 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 17:51:01.41 -05:18:50.4: 12.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.79 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4175310297408867328,2461239.8826,11.60,0.05,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 4175310297408867328 20260718.3826 11.60CV 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 07 18.3826 2461239.8826 12.05 17:57:30.07 -03:57:31.1
23.13507 10.11068 galactic Ser Second-epoch detections are separated by 0.9" and 7.3 pix
The object was found in VSX 2" ASASSN-V J175730.12-035732.9
Type: L
# Max. Min./Amp. JD0 Period
13.730 V 13.860 V
The object was not found in astcheck.
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 17:57:30.07 -03:57:31.1: 13.09 +/- 0.03 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 17:57:30.07 -03:57:31.1: 13.12 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.10 +/- 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!
TCP 2026 07 18.3826* 17 57 30.07 -03 57 31.1 12.1 U Ser 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 J175730.12-035732.9,2461239.8826,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J175730.12-035732.9 20260718.3826 12.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.3826 2461239.8826 11.76 17:50:17.15 -05:12:49.8
21.13626 11.08452 galactic Oph Second-epoch detections are separated by 0.3" and 7.1 pix
The object was found in VSX 1" ASASSN-V J175017.11-051251.0
Type: L
# Max. Min./Amp. JD0 Period
13.470 V 13.910 V
The object was not found in astcheck.
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 17:50:17.15 -05:12:49.8: 13.09 +/- 0.03 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 17:50:17.15 -05:12:49.8: 13.11 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.10 +/- 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 J175017.11-051251.0,2461239.8826,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J175017.11-051251.0 20260718.3826 11.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.3826 2461239.8826 11.50 18:03:08.91 -03:46:06.1
23.98307 8.96129 galactic Ser Second-epoch detections are separated by 0.7" and 7.1 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 4177258288415910016 | 18:03:08.94 -03:46:06.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.910+/-0.037 (M)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 18:03:08.91 -03:46:06.1: 12.69 +/- 0.02 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 18:03:08.91 -03:46:06.1: 12.70 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.70 +/- 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!
TCP 2026 07 18.3826* 18 03 08.91 -03 46 06.1 11.5 U Ser 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
Gaia DR3 4177258288415910016,2461239.8826,11.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4177258288415910016 20260718.3826 11.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.3826 2461239.8826 11.90 17:50:42.72 -05:32:38.6
20.89443 10.83167 galactic Oph Second-epoch detections are separated by 1.4" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J267.6777-05.5445 | 17:50:42.65 -05:32:40.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.432+/-0.045 (Very red! L if it's a dwarf)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 17:50:42.72 -05:32:38.6: 13.08 +/- 0.03 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 17:50:42.72 -05:32:38.6: 13.09 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J267.6777-05.5445,2461239.8826,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J267.6777-05.5445 20260718.3826 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.3826 2461239.8826 12.24 17:50:55.19 -05:16:44.8
21.15595 10.91482 galactic Oph Second-epoch detections are separated by 1.6" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 17:50:55.19 -05:16:44.8 (user input) | T | P | (position from user input) J-Ks=1.067+/-0.036 (M)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 17:50:55.19 -05:16:44.8: 13.52 +/- 0.04 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 17:50:55.19 -05:16:44.8: 13.37 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.44 +/- 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,2461239.8826,12.24,0.05,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 20260718.3826 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.3826 2461239.8826 12.22 17:51:07.00 -04:52:49.7
21.53554 11.06469 galactic Oph Second-epoch detections are separated by 1.3" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J267.7842-04.8789 | 17:51:07.00 -04:52:49.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.134+/-0.035 (M)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 17:51:07.00 -04:52:49.7: 13.29 +/- 0.03 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 17:51:07.00 -04:52:49.7: 13.34 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.32 +/- 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
ATO J267.7842-04.8789,2461239.8826,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J267.7842-04.8789 20260718.3826 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.3826 2461239.8826 12.24 17:51:53.37 -05:17:18.0
21.26664 10.69910 galactic Oph Second-epoch detections are separated by 2.3" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J267.9717-05.2885 | 17:51:53.23 -05:17:18.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.426+/-0.029 (Very red! L if it's a dwarf)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 17:51:53.37 -05:17:18.0: 13.30 +/- 0.04 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 17:51:53.37 -05:17:18.0: 13.33 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.31 +/- 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
ATO J267.9717-05.2885,2461239.8826,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J267.9717-05.2885 20260718.3826 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.3826 2461239.8826 11.21 18:06:24.46 -04:10:50.3
24.00406 8.05012 galactic Ser Second-epoch detections are separated by 0.8" and 7.1 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 4174189585821912960 | 18:06:24.48 -04:10:50.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K5 (LAMOST DR5) J-Ks=0.728+/-0.038 (K)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 18:06:24.46 -04:10:50.3: 12.30 +/- 0.01 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 18:06:24.46 -04:10:50.3: 12.35 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.33 +/- 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!
TCP 2026 07 18.3826* 18 06 24.46 -04 10 50.3 11.2 U Ser 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
Gaia DR3 4174189585821912960,2461239.8826,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4174189585821912960 20260718.3826 11.21CV 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 07 18.3826 2461239.8826 12.25 18:03:39.14 -03:45:13.0
24.05638 8.85752 galactic Ser Second-epoch detections are separated by 1.0" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:03:39.14 -03:45:13.0 (user input) | T | P | (position from user input) J-Ks=1.538+/-0.035 (Very red! L if it's a dwarf)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 18:03:39.14 -03:45:13.0: 13.76 +/- 0.05 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 18:03:39.14 -03:45:13.0: 13.74 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.75 +/- 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!
TCP 2026 07 18.3826* 18 03 39.14 -03 45 13.0 12.2 U Ser 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
target,2461239.8826,12.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.3826 12.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.3826 2461239.8826 12.19 17:52:01.09 -05:34:53.2
21.02142 10.52926 galactic Oph Second-epoch detections are separated by 8.8" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 17:52:01.09 -05:34:53.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 17:52:01.09 -05:34:53.2: 13.20 +/- 0.03 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 17:52:01.09 -05:34:53.2: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.8826,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.3826 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.3826 2461239.8826 11.94 17:49:21.15 -05:12:27.5
21.02695 11.29076 galactic Oph Second-epoch detections are separated by 1.2" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J267.3405-05.2172 | 17:49:21.13 -05:12:28.0 (Gaia DR3) | NSINE (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.918+/-0.030 (M)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 17:49:21.15 -05:12:27.5: 12.97 +/- 0.03 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 17:49:21.15 -05:12:27.5: 12.93 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J267.3405-05.2172,2461239.8826,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J267.3405-05.2172 20260718.3826 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.3826 2461239.8826 12.01 17:57:30.49 -04:05:39.9
23.01470 10.04441 galactic Oph Second-epoch detections are separated by 0.7" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4177372328388208512 | 17:57:30.47 -04:05:41.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.320+/-0.031 (Very red! L if it's a dwarf)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 17:57:30.49 -04:05:39.9: 12.97 +/- 0.03 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 17:57:30.49 -04:05:39.9: 12.99 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4177372328388208512,2461239.8826,12.01,0.05,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 4177372328388208512 20260718.3826 12.01CV 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 07 18.3826 2461239.8826 11.16 18:03:11.48 -04:15:12.6
23.55574 8.72216 galactic Oph Second-epoch detections are separated by 1.0" and 7.1 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 4174222571169906816 | 18:03:11.48 -04:15:12.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.857+/-0.035 (M)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 18:03:11.48 -04:15:12.6: 12.58 +/- 0.02 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 18:03:11.48 -04:15:12.6: 12.57 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.58 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4174222571169906816,2461239.8826,11.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4174222571169906816 20260718.3826 11.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.3826 2461239.8826 10.12 18:05:05.96 -04:10:39.2
23.85110 8.33909 galactic Ser Second-epoch detections are separated by 0.5" and 7.2 pix
The object was found in VSX 1" ASAS J180505-0410.5
Type: ROT
# Max. Min./Amp. JD0 Period
11.292 V Y 0.135 V 2.660000000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 18:05:05.96 -04:10:39.2: 11.18 +/- 0.00 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 18:05:05.96 -04:10:39.2: 11.21 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.20 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 18.3826* 18 05 05.96 -04 10 39.2 10.1 U Ser 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
ASAS J180505-0410.5,2461239.8826,10.12,0.05,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 J180505-0410.5 20260718.3826 10.12CV 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 07 18.3826 2461239.8826 11.51 18:06:30.59 -04:21:59.1
23.85085 7.93993 galactic Ser Second-epoch detections are separated by 0.6" and 7.1 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 4174173853358212992 | 18:06:30.57 -04:21:58.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.763+/-0.036 (K)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 18:06:30.59 -04:21:59.1: 12.59 +/- 0.02 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 18:06:30.59 -04:21:59.1: 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!
TCP 2026 07 18.3826* 18 06 30.59 -04 21 59.1 11.5 U Ser 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
Gaia DR3 4174173853358212992,2461239.8826,11.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4174173853358212992 20260718.3826 11.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.3826 2461239.8826 11.93 18:03:52.10 -03:49:56.7
24.01188 8.77278 galactic Ser Second-epoch detections are separated by 1.5" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:03:52.10 -03:49:56.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 18:03:52.10 -03:49:56.7: 13.43 +/- 0.04 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 18:03:52.10 -03:49:56.7: 13.44 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.44 +/- 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!
TCP 2026 07 18.3826* 18 03 52.10 -03 49 56.7 11.9 U Ser 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
target,2461239.8826,11.93,0.05,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 20260718.3826 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.3826 2461239.8826 11.85 17:49:40.32 -05:06:09.9
21.15982 11.27204 galactic Oph Second-epoch detections are separated by 1.8" and 7.1 pix
The object was found in VSX19" Gaia DR3 4175376714784915584
Type: L
# Max. Min./Amp. JD0 Period
18.200 G 18.440 G
ATTENTION: measured mag 11.85 is 6.3 mag brighter than the VSX record maximum brightness 18.20 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 17:49:40.32 -05:06:09.9: 12.91 +/- 0.03 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 17:49:40.32 -05:06:09.9: 12.94 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4175376714784915584,2461239.8826,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4175376714784915584 20260718.3826 11.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.3826 2461239.8826 11.55 18:07:16.51 -04:55:49.2
23.44033 7.50532 galactic Ser Second-epoch detections are separated by 0.9" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J271.8236-04.9289 | 18:07:16.51 -04:55:49.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.722+/-0.033 (K)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 18:07:16.51 -04:55:49.2: 12.54 +/- 0.02 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 18:07:16.51 -04:55:49.2: 12.58 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.56 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 18.3826* 18 07 16.51 -04 55 49.2 11.6 U Ser 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
ATO J271.8236-04.9289,2461239.8826,11.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J271.8236-04.9289 20260718.3826 11.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.3826 2461239.8826 12.25 17:51:45.65 -05:00:36.6
21.49879 10.86157 galactic Oph Second-epoch detections are separated by 2.7" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J267.9402-05.0103 | 17:51:45.67 -05:00:37.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.433+/-0.029 (Very red! L if it's a dwarf)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 17:51:45.65 -05:00:36.6: 13.25 +/- 0.04 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 17:51:45.65 -05:00:36.6: 13.25 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.25 +/- 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
ATO J267.9402-05.0103,2461239.8826,12.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J267.9402-05.0103 20260718.3826 12.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.3826 2461239.8826 11.96 17:49:56.07 -03:38:25.6
22.49956 11.92033 galactic Oph Second-epoch detections are separated by 0.7" and 6.9 pix
The object was found in VSX 0" ASASSN-V J174956.03-033825.6
Type: L
# Max. Min./Amp. JD0 Period
13.490 V 13.870 V
The object was not found in astcheck.
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 17:49:56.07 -03:38:25.6: 13.25 +/- 0.03 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 17:49:56.07 -03:38:25.6: 13.34 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.29 +/- 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 J174956.03-033825.6,2461239.8826,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J174956.03-033825.6 20260718.3826 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.3826 2461239.8826 12.19 17:49:20.81 -04:42:55.0
21.46567 11.53052 galactic Oph Second-epoch detections are separated by 1.6" and 7.0 pix
The object was found in VSX 1" ASASSN-V J174920.80-044256.2
Type: L
# Max. Min./Amp. JD0 Period
13.620 V 13.920 V
The object was not found in astcheck.
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 17:49:20.81 -04:42:55.0: 13.21 +/- 0.03 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 17:49:20.81 -04:42:55.0: 13.21 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.21 +/- 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 J174920.80-044256.2,2461239.8826,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J174920.80-044256.2 20260718.3826 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.3826 2461239.8826 9.66 18:04:49.07 -04:19:33.8
23.68532 8.33068 galactic Ser Second-epoch detections are separated by 0.2" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4174206529469436288 | 18:04:49.09 -04:19:33.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.403+/-0.033 (G)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 18:04:49.07 -04:19:33.8: 10.72 +/- 0.00 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 18:04:49.07 -04:19:33.8: 10.74 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.73 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 18.3826* 18 04 49.07 -04 19 33.8 9.7 U Ser 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
Gaia DR3 4174206529469436288,2461239.8826,9.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4174206529469436288 20260718.3826 9.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.3826 2461239.8826 12.04 17:50:01.66 -05:16:03.9
21.05646 11.11461 galactic Oph Second-epoch detections are separated by 3.9" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 17:50:01.66 -05:16:03.9 (user input) | T | P | (position from user input) J-Ks=1.283+/-0.032 (Very red! L if it's a dwarf)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 17:50:01.66 -05:16:03.9: 13.38 +/- 0.04 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 17:50:01.66 -05:16:03.9: 13.37 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.38 +/- 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,2461239.8826,12.04,0.05,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
target 20260718.3826 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 07 18.3826 2461239.8826 12.35 17:49:47.90 -05:14:01.6
21.05853 11.18102 galactic Oph Second-epoch detections are separated by 1.3" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J267.4497-05.2339 | 17:49:47.90 -05:14:01.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.041+/-0.032 (M)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 17:49:47.90 -05:14:01.6: 13.59 +/- 0.05 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 17:49:47.90 -05:14:01.6: 13.58 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.59 +/- 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
ATO J267.4497-05.2339,2461239.8826,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J267.4497-05.2339 20260718.3826 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.3826 2461239.8826 11.31 17:51:56.01 -05:28:59.2
21.09857 10.59530 galactic Oph Second-epoch detections are separated by 1.6" and 6.9 pix
The object was found in VSX 3" NSVS 13782617
Type: L
# Max. Min./Amp. JD0 Period
10.450 R1 10.900 R1
The object was not found in astcheck.
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 17:51:56.01 -05:28:59.2: 12.50 +/- 0.02 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 17:51:56.01 -05:28:59.2: 12.49 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.49 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 13782617,2461239.8826,11.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 13782617 20260718.3826 11.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.3826 2461239.8826 10.97 18:03:05.60 -03:37:32.6
24.10373 9.04087 galactic Ser Second-epoch detections are separated by 0.7" and 7.3 pix
The object was found in VSX 1" ASAS J180306-0337.5
Type: ROT
# Max. Min./Amp. JD0 Period
12.033 V Y 0.090 V 2.592000000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 18:03:05.60 -03:37:32.6: 11.94 +/- 0.01 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 18:03:05.60 -03:37:32.6: 11.98 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.96 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 18.3826* 18 03 05.60 -03 37 32.6 11.0 U Ser 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
ASAS J180306-0337.5,2461239.8826,10.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J180306-0337.5 20260718.3826 10.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.3826 2461239.8826 10.94 17:57:36.71 -04:06:20.3
23.01720 10.01633 galactic Oph Second-epoch detections are separated by 0.8" and 7.1 pix
The object was found in VSX 1" ASASSN-V J175736.71-040621.7
Type: SRS
# Max. Min./Amp. JD0 Period
12.570 V 12.690 V 2457070.12200 21.425000000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 17:57:36.71 -04:06:20.3: 11.94 +/- 0.01 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 17:57:36.71 -04:06:20.3: 11.95 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.95 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J175736.71-040621.7,2461239.8826,10.94,0.05,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
ASASSN-V J175736.71-040621.7 20260718.3826 10.94CV 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 07 18.3826 2461239.8826 10.88 18:06:36.82 -04:58:13.0
23.32618 7.63156 galactic Ser Second-epoch detections are separated by 0.9" and 7.0 pix
The object was found in VSX 3" ASASSN-V J180636.78-045815.6
Type: SR
# Max. Min./Amp. JD0 Period
13.940 g Y 0.200 g 2458359.64600 437.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 18:06:36.82 -04:58:13.0: 11.91 +/- 0.01 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 18:06:36.82 -04:58:13.0: 11.90 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.91 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 18.3826* 18 06 36.82 -04 58 13.0 10.9 U Ser 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 J180636.78-045815.6,2461239.8826,10.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J180636.78-045815.6 20260718.3826 10.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.3826 2461239.8826 11.93 18:01:52.77 -03:53:49.4
23.71650 9.17916 galactic Ser Second-epoch detections are separated by 1.2" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:01:52.77 -03:53:49.4 (user input) | T | P | (position from user input) J-Ks=0.443+/-0.031 (G)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 18:01:52.77 -03:53:49.4: 13.18 +/- 0.03 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 18:01:52.77 -03:53:49.4: 13.27 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.23 +/- 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!
TCP 2026 07 18.3826* 18 01 52.77 -03 53 49.4 11.9 U Ser 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
target,2461239.8826,11.93,0.05,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 20260718.3826 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.3826 2461239.8826 12.11 17:50:57.28 -06:07:31.6
20.40710 10.49656 galactic Oph Second-epoch detections are separated by 1.9" and 7.1 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 4175009855855141760 | 17:50:57.19 -06:07:32.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.355+/-0.040 (Very red! L if it's a dwarf)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 17:50:57.28 -06:07:31.6: 13.18 +/- 0.04 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 17:50:57.28 -06:07:31.6: 13.20 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.19 +/- 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 4175009855855141760,2461239.8826,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4175009855855141760 20260718.3826 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.3826 2461239.8826 12.06 17:51:02.70 -06:05:04.9
20.45442 10.49675 galactic Oph Second-epoch detections are separated by 2.1" and 7.4 pix
The object was found in VSX 1" ASASSN-V J175102.69-060505.4
Type: SR
# Max. Min./Amp. JD0 Period
13.530 V 13.660 V 2457813.86300 36.100000000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 17:51:02.70 -06:05:04.9: 13.14 +/- 0.03 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 17:51:02.70 -06:05:04.9: 13.28 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.20 +/- 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 J175102.69-060505.4,2461239.8826,12.06,0.05,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 J175102.69-060505.4 20260718.3826 12.06CV 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 07 18.3826 2461239.8826 10.87 17:49:52.86 -05:15:34.9
21.04559 11.15045 galactic Oph Second-epoch detections are separated by 0.6" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J267.4751-05.2687 | 17:49:52.77 -05:15:36.0 (Gaia DR3) | LPV (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.304+/-0.026 (Very red! L if it's a dwarf)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 17:49:52.86 -05:15:34.9: 11.81 +/- 0.01 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 17:49:52.86 -05:15:34.9: 11.78 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.79 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J267.4751-05.2687,2461239.8826,10.87,0.05,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
ATO J267.4751-05.2687 20260718.3826 10.87CV 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 07 18.3826 2461239.8826 12.38 17:49:26.20 -05:07:05.6
21.11706 11.31580 galactic Oph Second-epoch detections are separated by 3.1" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J267.3616-05.1209 | 17:49:26.20 -05:07:05.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.200+/-0.032 (M)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 17:49:26.20 -05:07:05.6: 13.53 +/- 0.04 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 17:49:26.20 -05:07:05.6: 13.54 +/- 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
ATO J267.3616-05.1209,2461239.8826,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J267.3616-05.1209 20260718.3826 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.3826 2461239.8826 12.34 17:56:44.38 -03:52:15.4
23.12140 10.31944 galactic Ser Second-epoch detections are separated by 4.2" and 6.7 pix
The object was found in VSX 1" ASASSN-V J175644.37-035214.3
Type: L:
# Max. Min./Amp. JD0 Period
14.470 V 14.830 V
The object was found in astcheck.14721 2000 CW91 -89 -268 283 17.1 -0 0
NOTE: the measured brightness disagrees with the predicted asteroid brightness, but the matched variable star above likely accounts for this object.
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 17:56:44.38 -03:52:15.4: 13.55 +/- 0.04 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 17:56:44.38 -03:52:15.4: 13.58 +/- 0.04 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!
TCP 2026 07 18.3826* 17 56 44.38 -03 52 15.4 12.3 U Ser 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 J175644.37-035214.3,2461239.8826,12.34,0.05,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
ASASSN-V J175644.37-035214.3 20260718.3826 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 07 18.3826 2461239.8826 12.53 18:04:07.13 -03:39:39.4
24.19468 8.79873 galactic Ser Second-epoch detections are separated by 0.6" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:04:07.13 -03:39:39.4 (user input) | T | P | (position from user input) J-Ks=0.661+/-0.035 (K)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 18:04:07.13 -03:39:39.4: 14.01 +/- 0.06 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 18:04:07.13 -03:39:39.4: 14.06 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.04 +/- 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!
TCP 2026 07 18.3826* 18 04 07.13 -03 39 39.4 12.5 U Ser 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
target,2461239.8826,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.3826 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.3826 2461239.8826 11.76 18:03:46.30 -03:47:21.9
24.03869 8.81436 galactic Ser Second-epoch detections are separated by 0.3" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:03:46.30 -03:47:21.9 (user input) | T | P | (position from user input) J-Ks=0.675+/-0.032 (K)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 18:03:46.30 -03:47:21.9: 13.12 +/- 0.03 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 18:03:46.30 -03:47:21.9: 13.08 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.10 +/- 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!
TCP 2026 07 18.3826* 18 03 46.30 -03 47 21.9 11.8 U Ser 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
target,2461239.8826,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.3826 11.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.3826 2461239.8826 12.03 18:03:02.40 -03:37:43.0
24.09478 9.05123 galactic Ser Second-epoch detections are separated by 1.2" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:03:02.40 -03:37:43.0 (user input) | T | P | (position from user input) J-Ks=0.626+/-0.030 (K)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 18:03:02.40 -03:37:43.0: 13.13 +/- 0.03 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 18:03:02.40 -03:37:43.0: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 18.3826* 18 03 02.40 -03 37 43.0 12.0 U Ser 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
target,2461239.8826,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.3826 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.3826 2461239.8826 11.80 17:52:10.70 -05:10:57.0
21.39630 10.68730 galactic Oph Second-epoch detections are separated by 1.7" and 7.1 pix
The object was found in VSX 2" ASASSN-V J175210.59-051058.5
Type: SR
# Max. Min./Amp. JD0 Period
13.760 V 14.030 V 2457631.81100 50.590000000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 17:52:10.70 -05:10:57.0: 13.11 +/- 0.03 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 17:52:10.70 -05:10:57.0: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J175210.59-051058.5,2461239.8826,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J175210.59-051058.5 20260718.3826 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.3826 2461239.8826 12.09 17:48:26.50 -04:48:54.5
21.26499 11.67947 galactic Oph Second-epoch detections are separated by 2.4" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 17:48:26.50 -04:48:54.5 (user input) | T | P | (position from user input) J-Ks=0.924+/-0.036 (M)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 17:48:26.50 -04:48:54.5: 13.12 +/- 0.03 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 17:48:26.50 -04:48:54.5: 13.17 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.8826,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.3826 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.3826 2461239.8826 12.14 17:48:57.12 -04:46:05.6
21.36978 11.59098 galactic Oph Second-epoch detections are separated by 1.1" and 7.3 pix
The object was not found in VSX
The object was found in ASASSN-V 1" ASASSN-V J174857.05-044606.0
Type: SR
MeanMag 13.55 m Amp. 0.09 m Period 18.5236352 d
The object was not found in astcheck.
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 17:48:57.12 -04:46:05.6: 13.11 +/- 0.03 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 17:48:57.12 -04:46:05.6: 13.09 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.10 +/- 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
VARIABLE_NAME,2461239.8826,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260718.3826 12.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.3826 2461239.8826 10.63 18:04:01.91 -04:01:58.3
23.85272 8.64206 galactic Oph Second-epoch detections are separated by 0.2" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4174235181194182400 | 18:04:01.88 -04:01:58.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A2IV (LAMOST DR5) J-Ks=0.332+/-0.031 (G)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 18:04:01.91 -04:01:58.3: 11.72 +/- 0.01 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 18:04:01.91 -04:01:58.3: 11.74 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.73 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4174235181194182400,2461239.8826,10.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4174235181194182400 20260718.3826 10.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.3826 2461239.8826 10.84 18:06:14.50 -04:03:49.5
24.08841 8.14178 galactic Ser Second-epoch detections are separated by 0.4" and 7.1 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 4174194567983226496 | 18:06:14.53 -04:03:49.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.500+/-0.049 (K)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 18:06:14.50 -04:03:49.5: 11.71 +/- 0.01 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 18:06:14.50 -04:03:49.5: 11.67 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.69 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 18.3826* 18 06 14.50 -04 03 49.5 10.8 U Ser 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
Gaia DR3 4174194567983226496,2461239.8826,10.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4174194567983226496 20260718.3826 10.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461200.78210244 09.06.2026 06:46:03.651 /data_ssd/NMW-TexasTech/reference_imgs/Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits
First image: 2461200.78210244 09.06.2026 06:46:03.651 /data_ssd/NMW-TexasTech/reference_imgs/Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits
Last image: 2461239.88284087 18.07.2026 09:11:07.451 /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Ser-07-Q2b1x1_041149_TTUQ2b1x1_928637_e4bqkijR/fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.76
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: 4 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): 8156
Objects passed selection criteria: 8107
Measurements per detected object (mean, median, min, max): 2.1 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.1 2.0 2 4
Average stars detected per image: 4555.5
Average stars matched: 4295 (94.2816 %)
Memory usage VmPeak: 117784 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Jul 17 15:05:04 CDT 2026
VaST build number 1.0rc89-157-gbf7d0e63
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-17)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Jul 18 08:29:35 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: 2461200.78210244 09.06.2026 06:46:03.651 /data_ssd/NMW-TexasTech/reference_imgs/Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits
First image: 2461200.78210244 09.06.2026 06:46:03.651 /data_ssd/NMW-TexasTech/reference_imgs/Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits
Last image: 2461239.88284087 18.07.2026 09:11:07.451 /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Ser-07-Q2b1x1_041149_TTUQ2b1x1_928637_e4bqkijR/fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 52
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.36
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: 15 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): 81195
Objects passed selection criteria: 80934
Measurements per detected object (mean, median, min, max): 2.1 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.1 2.0 2 4
Average stars detected per image: 47090.2
Average stars matched: 43970.8 (93.3755 %)
Memory usage VmPeak: 188164 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Jul 17 15:05:04 CDT 2026
VaST build number 1.0rc89-157-gbf7d0e63
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-17)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Jul 18 08:33:03 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits /data_ssd/NMW-TexasTech/reference_imgs/Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Ser-07-Q2b1x1_041149_TTUQ2b1x1_928637_e4bqkijR/fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Ser-07-Q2b1x1_041149_TTUQ2b1x1_928637_e4bqkijR/fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits
SExtractor catalog cache: saved Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits.cat to cache
SExtractor catalog cache: saved Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.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/Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits /data_ssd/NMW-TexasTech/reference_imgs/Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Ser-07-Q2b1x1_041149_TTUQ2b1x1_928637_e4bqkijR/fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Ser-07-Q2b1x1_041149_TTUQ2b1x1_928637_e4bqkijR/fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.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: 2461239.88234881
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits exists and is non-empty
Saving wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits to local_wcs_cache/
'wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits' -> 'local_wcs_cache/wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits'
wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits exists and is non-empty
Saving wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits to local_wcs_cache/
'wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits' -> 'local_wcs_cache/wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits'
wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits exists and is non-empty
Saving wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits to local_wcs_cache/
'wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits' -> 'local_wcs_cache/wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits'
wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits exists and is non-empty
Saving wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits to local_wcs_cache/
'wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits' -> 'local_wcs_cache/wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits (1st reference image)
verification OK: wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits
Image size: 937.1'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: 17:59:59.071 -01:58:35.72 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_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits (1st new image)
verification OK: wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits
Image size: 937.7'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: 18:00:00.527 -02:00:09.18 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 17:59:59.071 -01:58:35.72
Second-epoch image center 18:00:00.527 -02:00:09.18
Angular distance between the image centers 0.0267 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits (2nd new image)
verification OK: wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits
Image size: 937.7'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: 18:00:03.274 -01:59:59.48 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 17:59:59.071 -01:58:35.72
Second-epoch image center 18:00:03.274 -01:59:59.48
Angular distance between the image centers 0.0291 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 18:00:00.527 -02:00:09.18
Second-epoch second image center 18:00:03.274 -01:59:59.48
Angular distance between the image centers 0.01175 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits &> /tmp/tmp.xN0Kzy1IiS
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits &> /tmp/tmp.GyOlf6v4tx
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Ser-07-Q2b1x1_041149_TTUQ2b1x1_928637_e4bqkijR/fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits &> /tmp/tmp.eZg8plqEHH
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Ser-07-Q2b1x1_041149_TTUQ2b1x1_928637_e4bqkijR/fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Ser-07-Q2b1x1_041149_TTUQ2b1x1_928637_e4bqkijR/fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits &> /tmp/tmp.GxrRiHT960
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Ser-07-Q2b1x1_041149_TTUQ2b1x1_928637_e4bqkijR/fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits
Calibrating the magnitude scale
Found non-empty wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.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_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits and wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits and wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits.wcscat
Found non-empty wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits and wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits.wcscat
The reference image (wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits) and catalog (wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits.wcscat) found
'wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits.wcscat' -> 'wcsmag.cat'
Read 10373 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 262.1403 to 277.8780 deg, Dec -7.2432 to +3.2893 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 262.1403 to 277.8780 deg, Dec -7.2432 to 3.2893 deg
Loaded 5310 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): 4363 out of 4602 total matches.
Matched with Tycho-2 4602 out of 10373 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.731800
a=0.000000 b=1.000000 c=22.731800
From vast_summary.log: estimated ref. image limiting mag.: -7.76
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.97
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.97
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 10373 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 262.1403 to 277.8780 deg, Dec -7.2432 to +3.2893 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 262.1403 to 277.8780 deg, Dec -7.2432 to 3.2893 deg
Loaded 5310 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): 4363 out of 4602 total matches.
Matched with Tycho-2 4602 out of 10373 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits:
Forced-photometry filter: calibrated wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits -> calib.txt_param_ref_wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits (aperture=6.1)
Read 10954 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 262.1474 to 277.8778 deg, Dec -7.2480 to +3.2694 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 262.1474 to 277.8778 deg, Dec -7.2480 to 3.2694 deg
Loaded 5284 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): 4374 out of 4605 total matches.
Matched with Tycho-2 4605 out of 10954 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits:
Forced-photometry filter: calibrated wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits -> calib.txt_param_ref_wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits (aperture=6.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits
2.2 pix Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits
2.3 pix fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits
2.3 pix fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits
2.2 pix wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits
2.2 pix wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits
Limiting magnitude estimates:
15.0 mag. Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits
15.0 mag. Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits
11.8 mag. fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits
12.5 mag. fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits
All-image limiting magnitude estimate: 11.8 (SNR ) 10.1 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.xN0Kzy1IiS (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_2026-07-18_CI_Ser-07-Q2b1x1_041149_TTUQ2b1x1_928637_e4bqkijR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits' -> 'wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits
WCS_IMAGE_NAME=wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits
WCS-calibrated image found: wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits
Checking if the catalog wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits.wcscat corresponding to the image wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits alredy exist and is non-empty...
Catalog wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits.wcscat corresponding to the image wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits
WCS catalog name: wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=711, bad_region=1882, passed=10373
Got 10373 stars (including 7894 good ones) from the SExtractor catalog wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits.wcscat
util/solve_plate_with_UCAC5 got 10373 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (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 413 to 468 (Dec -7.2 to 3.3)
Done reading UCAC5 zone files...
Matched 908 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 907 matched stars entering correct_measured_positions(), 896 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 907 matched stars entering correct_measured_positions(), 8527 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
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 413 to 468 (Dec -7.2 to 3.3)
Done reading UCAC5 zone files...
Matched 908 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 907 matched stars entering correct_measured_positions(), 8526 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 907 matched stars entering correct_measured_positions(), 8526 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 907 stars left (next iteration limit 997)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits N_match=907 sigma_overall_arcsec=0.477 sigma_q1_arcsec=0.442 sigma_q2_arcsec=0.546 sigma_q3_arcsec=0.451 sigma_q4_arcsec=0.493 n_q1=223 n_q2=101 n_q3=343 n_q4=240 worst_quadrant_to_overall_ratio=1.145
The image catalog is written to wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits -region wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.GyOlf6v4tx (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_2026-07-18_CI_Ser-07-Q2b1x1_041149_TTUQ2b1x1_928637_e4bqkijR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits' -> 'wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits
WCS_IMAGE_NAME=wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits
WCS-calibrated image found: wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits
Checking if the catalog wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits.wcscat corresponding to the image wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits alredy exist and is non-empty...
Catalog wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits.wcscat corresponding to the image wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits
WCS catalog name: wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=741, bad_region=1989, passed=10954
Got 10954 stars (including 8347 good ones) from the SExtractor catalog wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits.wcscat
util/solve_plate_with_UCAC5 got 10954 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (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 413 to 468 (Dec -7.2 to 3.3)
Done reading UCAC5 zone files...
Matched 907 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 906 matched stars entering correct_measured_positions(), 893 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 906 matched stars entering correct_measured_positions(), 9042 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
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 413 to 468 (Dec -7.2 to 3.3)
Done reading UCAC5 zone files...
Matched 907 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 906 matched stars entering correct_measured_positions(), 9042 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 906 matched stars entering correct_measured_positions(), 9042 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 906 stars left (next iteration limit 996)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits N_match=906 sigma_overall_arcsec=0.481 sigma_q1_arcsec=0.422 sigma_q2_arcsec=0.525 sigma_q3_arcsec=0.507 sigma_q4_arcsec=0.516 n_q1=224 n_q2=100 n_q3=346 n_q4=236 worst_quadrant_to_overall_ratio=1.091
The image catalog is written to wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits -region wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.eZg8plqEHH (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_2026-07-18_CI_Ser-07-Q2b1x1_041149_TTUQ2b1x1_928637_e4bqkijR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Ser-07-Q2b1x1_041149_TTUQ2b1x1_928637_e4bqkijR/fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Ser-07-Q2b1x1_041149_TTUQ2b1x1_928637_e4bqkijR/fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Ser-07-Q2b1x1_041149_TTUQ2b1x1_928637_e4bqkijR/fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Ser-07-Q2b1x1_041149_TTUQ2b1x1_928637_e4bqkijR/fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Ser-07-Q2b1x1_041149_TTUQ2b1x1_928637_e4bqkijR/fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.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_2026-07-18_CI_Ser-07-Q2b1x1_041149_TTUQ2b1x1_928637_e4bqkijR/fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits
WCS_IMAGE_NAME=wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits
WCS-calibrated image found: wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits
Checking if the catalog wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits.wcscat corresponding to the image wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits alredy exist and is non-empty...
Catalog wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits.wcscat corresponding to the image wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Ser-07-Q2b1x1_041149_TTUQ2b1x1_928637_e4bqkijR/fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits
WCS catalog name: wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=25, bad_region=67, passed=550
Got 550 stars (including 461 good ones) from the SExtractor catalog wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits.wcscat
util/solve_plate_with_UCAC5 got 550 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (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 413 to 468 (Dec -7.3 to 3.2)
Done reading UCAC5 zone files...
Matched 419 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 418 matched stars entering correct_measured_positions(), 380 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 418 matched stars entering correct_measured_positions(), 441 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
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 413 to 468 (Dec -7.3 to 3.2)
Done reading UCAC5 zone files...
Matched 419 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 417 matched stars entering correct_measured_positions(), 440 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Accuracy estimation diagnostic: 417 matched stars entering correct_measured_positions(), 439 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Excluding outliers - 417 stars left (next iteration limit 459)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits N_match=417 sigma_overall_arcsec=0.651 sigma_q1_arcsec=0.850 sigma_q2_arcsec=0.735 sigma_q3_arcsec=0.551 sigma_q4_arcsec=0.564 n_q1=157 n_q2=14 n_q3=113 n_q4=133 worst_quadrant_to_overall_ratio=1.306
The image catalog is written to wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Ser-07-Q2b1x1_041149_TTUQ2b1x1_928637_e4bqkijR/fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits -region wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.GxrRiHT960 (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_2026-07-18_CI_Ser-07-Q2b1x1_041149_TTUQ2b1x1_928637_e4bqkijR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Ser-07-Q2b1x1_041149_TTUQ2b1x1_928637_e4bqkijR/fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Ser-07-Q2b1x1_041149_TTUQ2b1x1_928637_e4bqkijR/fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Ser-07-Q2b1x1_041149_TTUQ2b1x1_928637_e4bqkijR/fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Ser-07-Q2b1x1_041149_TTUQ2b1x1_928637_e4bqkijR/fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Ser-07-Q2b1x1_041149_TTUQ2b1x1_928637_e4bqkijR/fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.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_2026-07-18_CI_Ser-07-Q2b1x1_041149_TTUQ2b1x1_928637_e4bqkijR/fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits
WCS_IMAGE_NAME=wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits
WCS-calibrated image found: wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits
Checking if the catalog wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits.wcscat corresponding to the image wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits alredy exist and is non-empty...
Catalog wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits.wcscat corresponding to the image wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Ser-07-Q2b1x1_041149_TTUQ2b1x1_928637_e4bqkijR/fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits
WCS catalog name: wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=18, bad_region=41, passed=442
Got 442 stars (including 384 good ones) from the SExtractor catalog wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits.wcscat
util/solve_plate_with_UCAC5 got 442 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (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 413 to 467 (Dec -7.3 to 3.2)
Done reading UCAC5 zone files...
Matched 348 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 347 matched stars entering correct_measured_positions(), 299 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 347 matched stars entering correct_measured_positions(), 352 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 467 (Dec -7.3 to 3.2)
Done reading UCAC5 zone files...
Matched 348 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 347 matched stars entering correct_measured_positions(), 348 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Accuracy estimation diagnostic: 347 matched stars entering correct_measured_positions(), 348 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Excluding outliers - 347 stars left (next iteration limit 381)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits N_match=347 sigma_overall_arcsec=0.703 sigma_q1_arcsec=0.894 sigma_q2_arcsec=0.708 sigma_q3_arcsec=0.560 sigma_q4_arcsec=0.749 n_q1=66 n_q2=15 n_q3=91 n_q4=175 worst_quadrant_to_overall_ratio=1.272
The image catalog is written to wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Ser-07-Q2b1x1_041149_TTUQ2b1x1_928637_e4bqkijR/fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits -region wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits sigma_overall=0.477 worst_q_ratio=1.145
ref2=Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits sigma_overall=0.481 worst_q_ratio=1.091
new1=fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits sigma_overall=0.651 worst_q_ratio=1.306
new2=fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits sigma_overall=0.703 worst_q_ratio=1.272
reference average sigma_overall=0.479 worst_q_ratio=1.118
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086_astrometric_residuals.png (907 matched stars from wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.43 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094_astrometric_residuals.png (906 matched stars from wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.43 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335_astrometric_residuals.png (417 matched stars from wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.59 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336_astrometric_residuals.png (347 matched stars from wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.63 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Ser-07-Q2b1x1_041149_TTUQ2b1x1_928637_e4bqkijR/wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits'
Saving fully-calibrated image wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Ser-07-Q2b1x1_041149_TTUQ2b1x1_928637_e4bqkijR/wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits'
Preparing the HTML report for the field Ser-07-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Ser-07-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits /data_ssd/NMW-TexasTech/reference_imgs/Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Ser-07-Q2b1x1_041149_TTUQ2b1x1_928637_e4bqkijR/fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Ser-07-Q2b1x1_041149_TTUQ2b1x1_928637_e4bqkijR/fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits
SExtractor catalog cache: saved Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits.cat to cache
SExtractor catalog cache: saved Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits /data_ssd/NMW-TexasTech/reference_imgs/Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Ser-07-Q2b1x1_041149_TTUQ2b1x1_928637_e4bqkijR/fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Ser-07-Q2b1x1_041149_TTUQ2b1x1_928637_e4bqkijR/fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits
Creating symlink local_wcs_cache/wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits
Creating symlink local_wcs_cache/wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits
Creating symlink local_wcs_cache/wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.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_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits exists and is non-empty
wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits exists and is non-empty
wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits exists and is non-empty
wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits (1st reference image)
verification OK: wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits
Image size: 937.1'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: 17:59:59.071 -01:58:35.72 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_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits (1st new image)
verification OK: wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits
Image size: 937.7'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: 18:00:00.527 -02:00:09.18 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 17:59:59.071 -01:58:35.72
Second-epoch image center 18:00:00.527 -02:00:09.18
Angular distance between the image centers 0.0267 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits (2nd new image)
verification OK: wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits
Image size: 937.7'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: 18:00:03.274 -01:59:59.48 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 17:59:59.071 -01:58:35.72
Second-epoch image center 18:00:03.274 -01:59:59.48
Angular distance between the image centers 0.0291 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 18:00:00.527 -02:00:09.18
Second-epoch second image center 18:00:03.274 -01:59:59.48
Angular distance between the image centers 0.01175 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits &> /tmp/tmp.8p8RblatDM
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits &> /tmp/tmp.tunyAYsoRj
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Ser-07-Q2b1x1_041149_TTUQ2b1x1_928637_e4bqkijR/fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits &> /tmp/tmp.boIAOVpOLL
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Ser-07-Q2b1x1_041149_TTUQ2b1x1_928637_e4bqkijR/fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Ser-07-Q2b1x1_041149_TTUQ2b1x1_928637_e4bqkijR/fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits &> /tmp/tmp.PXnmhj2PYT
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Ser-07-Q2b1x1_041149_TTUQ2b1x1_928637_e4bqkijR/fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits
Calibrating the magnitude scale
Found non-empty wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.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_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits and wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits and wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits.wcscat
Found non-empty wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits and wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits.wcscat
The reference image (wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits) and catalog (wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits.wcscat) found
'wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits.wcscat' -> 'wcsmag.cat'
Read 102040 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 262.1381 to 277.8815 deg, Dec -7.2435 to +3.2926 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 262.1381 to 277.8815 deg, Dec -7.2435 to 3.2926 deg
Loaded 5314 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): 3858 out of 4714 total matches.
Matched with Tycho-2 4714 out of 102040 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.555550
a=0.000000 b=1.000000 c=22.555550
From vast_summary.log: estimated ref. image limiting mag.: -7.36
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.20
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.20
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 102040 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 262.1381 to 277.8815 deg, Dec -7.2435 to +3.2926 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 262.1381 to 277.8815 deg, Dec -7.2435 to 3.2926 deg
Loaded 5314 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): 3858 out of 4714 total matches.
Matched with Tycho-2 4714 out of 102040 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits:
Forced-photometry filter: calibrated wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits -> calib.txt_param_ref_wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits (aperture=4.4)
Read 105043 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 262.1455 to 277.8883 deg, Dec -7.2611 to +3.2742 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 262.1455 to 277.8883 deg, Dec -7.2611 to 3.2742 deg
Loaded 5300 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): 3841 out of 4697 total matches.
Matched with Tycho-2 4697 out of 105043 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits:
Forced-photometry filter: calibrated wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits -> calib.txt_param_ref_wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits (aperture=4.5)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 48 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits
2.1 pix Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits
2.3 pix fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits
2.2 pix fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits
2.0 pix wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits
2.1 pix wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits
Limiting magnitude estimates:
15.2 mag. Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits
15.2 mag. Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits
12.5 mag. fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits
12.9 mag. fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits
All-image limiting magnitude estimate: 12.5 (SNR ) 12.3 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.8p8RblatDM (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_2026-07-18_CI_Ser-07-Q2b1x1_041149_TTUQ2b1x1_928637_e4bqkijR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits' -> 'wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits
WCS_IMAGE_NAME=wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits
WCS-calibrated image found: wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits
Checking if the catalog wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits.wcscat corresponding to the image wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits alredy exist and is non-empty...
Catalog wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits.wcscat corresponding to the image wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits
WCS catalog name: wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=8553, bad_region=12678, passed=102031
Got 102031 stars (including 81731 good ones) from the SExtractor catalog wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits.wcscat
util/solve_plate_with_UCAC5 got 102031 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (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 413 to 468 (Dec -7.2 to 3.3)
Done reading UCAC5 zone files...
Matched 916 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 915 matched stars entering correct_measured_positions(), 904 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 915 matched stars entering correct_measured_positions(), 90177 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
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 413 to 468 (Dec -7.2 to 3.3)
Done reading UCAC5 zone files...
Matched 916 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 915 matched stars entering correct_measured_positions(), 90178 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 915 matched stars entering correct_measured_positions(), 90178 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 915 stars left (next iteration limit 1006)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits N_match=915 sigma_overall_arcsec=0.480 sigma_q1_arcsec=0.450 sigma_q2_arcsec=0.550 sigma_q3_arcsec=0.444 sigma_q4_arcsec=0.473 n_q1=233 n_q2=108 n_q3=343 n_q4=231 worst_quadrant_to_overall_ratio=1.146
The image catalog is written to wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits -region wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.tunyAYsoRj (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_2026-07-18_CI_Ser-07-Q2b1x1_041149_TTUQ2b1x1_928637_e4bqkijR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits' -> 'wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits
WCS_IMAGE_NAME=wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits
WCS-calibrated image found: wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits
Checking if the catalog wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits.wcscat corresponding to the image wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits alredy exist and is non-empty...
Catalog wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits.wcscat corresponding to the image wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits
WCS catalog name: wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=8912, bad_region=13384, passed=105035
Got 105035 stars (including 83689 good ones) from the SExtractor catalog wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits.wcscat
util/solve_plate_with_UCAC5 got 105035 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 914 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 913 matched stars entering correct_measured_positions(), 902 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 913 matched stars entering correct_measured_positions(), 92643 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 914 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 913 matched stars entering correct_measured_positions(), 92646 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 913 matched stars entering correct_measured_positions(), 92646 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 913 stars left (next iteration limit 1004)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits N_match=913 sigma_overall_arcsec=0.456 sigma_q1_arcsec=0.396 sigma_q2_arcsec=0.509 sigma_q3_arcsec=0.466 sigma_q4_arcsec=0.458 n_q1=231 n_q2=111 n_q3=340 n_q4=231 worst_quadrant_to_overall_ratio=1.117
The image catalog is written to wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits -region wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.boIAOVpOLL (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_2026-07-18_CI_Ser-07-Q2b1x1_041149_TTUQ2b1x1_928637_e4bqkijR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Ser-07-Q2b1x1_041149_TTUQ2b1x1_928637_e4bqkijR/fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Ser-07-Q2b1x1_041149_TTUQ2b1x1_928637_e4bqkijR/fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Ser-07-Q2b1x1_041149_TTUQ2b1x1_928637_e4bqkijR/fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Ser-07-Q2b1x1_041149_TTUQ2b1x1_928637_e4bqkijR/fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Ser-07-Q2b1x1_041149_TTUQ2b1x1_928637_e4bqkijR/fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.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_2026-07-18_CI_Ser-07-Q2b1x1_041149_TTUQ2b1x1_928637_e4bqkijR/fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits
WCS_IMAGE_NAME=wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits
WCS-calibrated image found: wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits
Checking if the catalog wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits.wcscat corresponding to the image wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits alredy exist and is non-empty...
Catalog wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits.wcscat corresponding to the image wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Ser-07-Q2b1x1_041149_TTUQ2b1x1_928637_e4bqkijR/fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits
WCS catalog name: wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=96, bad_region=558, passed=5101
Got 5101 stars (including 4456 good ones) from the SExtractor catalog wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits.wcscat
util/solve_plate_with_UCAC5 got 5101 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 908 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 905 matched stars entering correct_measured_positions(), 885 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 905 matched stars entering correct_measured_positions(), 4541 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 907 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 905 matched stars entering correct_measured_positions(), 4542 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Accuracy estimation diagnostic: 905 matched stars entering correct_measured_positions(), 4542 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Excluding outliers - 905 stars left (next iteration limit 995)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits N_match=905 sigma_overall_arcsec=0.707 sigma_q1_arcsec=0.748 sigma_q2_arcsec=0.791 sigma_q3_arcsec=0.578 sigma_q4_arcsec=0.767 n_q1=340 n_q2=30 n_q3=241 n_q4=294 worst_quadrant_to_overall_ratio=1.119
The image catalog is written to wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Ser-07-Q2b1x1_041149_TTUQ2b1x1_928637_e4bqkijR/fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits -region wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.PXnmhj2PYT (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_2026-07-18_CI_Ser-07-Q2b1x1_041149_TTUQ2b1x1_928637_e4bqkijR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Ser-07-Q2b1x1_041149_TTUQ2b1x1_928637_e4bqkijR/fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Ser-07-Q2b1x1_041149_TTUQ2b1x1_928637_e4bqkijR/fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Ser-07-Q2b1x1_041149_TTUQ2b1x1_928637_e4bqkijR/fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Ser-07-Q2b1x1_041149_TTUQ2b1x1_928637_e4bqkijR/fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Ser-07-Q2b1x1_041149_TTUQ2b1x1_928637_e4bqkijR/fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.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_2026-07-18_CI_Ser-07-Q2b1x1_041149_TTUQ2b1x1_928637_e4bqkijR/fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits
WCS_IMAGE_NAME=wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits
WCS-calibrated image found: wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits
Checking if the catalog wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits.wcscat corresponding to the image wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits alredy exist and is non-empty...
Catalog wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits.wcscat corresponding to the image wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Ser-07-Q2b1x1_041149_TTUQ2b1x1_928637_e4bqkijR/fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits
WCS catalog name: wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=90, bad_region=484, passed=4569
Got 4569 stars (including 4005 good ones) from the SExtractor catalog wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits.wcscat
util/solve_plate_with_UCAC5 got 4569 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 897 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 893 matched stars entering correct_measured_positions(), 871 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 893 matched stars entering correct_measured_positions(), 4101 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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 896 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 893 matched stars entering correct_measured_positions(), 4102 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Accuracy estimation diagnostic: 893 matched stars entering correct_measured_positions(), 4102 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Excluding outliers - 893 stars left (next iteration limit 982)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits N_match=893 sigma_overall_arcsec=0.721 sigma_q1_arcsec=0.834 sigma_q2_arcsec=0.909 sigma_q3_arcsec=0.609 sigma_q4_arcsec=0.698 n_q1=193 n_q2=42 n_q3=239 n_q4=419 worst_quadrant_to_overall_ratio=1.260
The image catalog is written to wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Ser-07-Q2b1x1_041149_TTUQ2b1x1_928637_e4bqkijR/fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits -region wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.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_2026-07-18_CI_Ser-07-Q2b1x1_041149_TTUQ2b1x1_928637_e4bqkijR/wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits
Saving fully-calibrated image wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.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_2026-07-18_CI_Ser-07-Q2b1x1_041149_TTUQ2b1x1_928637_e4bqkijR/wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits
Preparing the HTML report for the field Ser-07-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 18:03:08.91 -03:46:06.1: 12.69 +/- 0.02 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 17:51:07.00 -04:52:49.7: 13.29 +/- 0.03 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 17:50:42.72 -05:32:38.6: 13.08 +/- 0.03 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 17:51:01.41 -05:18:50.4: 12.77 +/- 0.02 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 18:06:24.46 -04:10:50.3: 12.30 +/- 0.01 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 17:50:17.15 -05:12:49.8: 13.09 +/- 0.03 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 17:51:53.37 -05:17:18.0: 13.30 +/- 0.04 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 18:07:13.64 -05:07:28.9: 12.92 +/- 0.03 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 17:57:30.07 -03:57:31.1: 13.09 +/- 0.03 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 17:50:55.19 -05:16:44.8: 13.52 +/- 0.04 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 17:51:07.00 -04:52:49.7: 13.34 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.03
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 18:03:08.91 -03:46:06.1: 12.70 +/- 0.02 detection
Forced photometry filter KEPT candidate at 17:51:07.00 -04:52:49.7: ref_mag=13.32 +/- 0.03 new_mean_mag=12.2490 delta=1.07 (need > 0.90)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 17:51:53.37 -05:17:18.0: 13.33 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.01
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 17:50:17.15 -05:12:49.8: 13.11 +/- 0.03 detection
Forced photometry filter KEPT candidate at 18:03:08.91 -03:46:06.1: ref_mag=12.70 +/- 0.01 new_mean_mag=11.5054 delta=1.19 (need > 0.90)
Forced photometry reference-image weighted average: 13.31 +/- 0.03
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 17:50:55.19 -05:16:44.8: 13.37 +/- 0.04 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 17:50:42.72 -05:32:38.6: 13.09 +/- 0.03 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 17:51:01.41 -05:18:50.4: 12.81 +/- 0.02 detection
Forced photometry filter KEPT candidate at 17:51:53.37 -05:17:18.0: ref_mag=13.31 +/- 0.03 new_mean_mag=12.2418 delta=1.07 (need > 0.90)
Forced photometry reference-image weighted average: 13.10 +/- 0.02
Forced photometry reference-image weighted average: 13.44 +/- 0.03
Forced photometry reference-image weighted average: 13.08 +/- 0.02
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 18:06:24.46 -04:10:50.3: 12.35 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.79 +/- 0.02
Forced photometry filter KEPT candidate at 17:50:17.15 -05:12:49.8: ref_mag=13.10 +/- 0.02 new_mean_mag=11.7605 delta=1.34 (need > 0.90)
Forced photometry filter KEPT candidate at 17:50:55.19 -05:16:44.8: ref_mag=13.44 +/- 0.03 new_mean_mag=12.2447 delta=1.19 (need > 0.90)
Forced photometry filter KEPT candidate at 17:50:42.72 -05:32:38.6: ref_mag=13.08 +/- 0.02 new_mean_mag=11.9114 delta=1.17 (need > 0.90)
Forced photometry filter KEPT candidate at 17:51:01.41 -05:18:50.4: ref_mag=12.79 +/- 0.02 new_mean_mag=11.6052 delta=1.18 (need > 0.90)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 17:57:30.07 -03:57:31.1: 13.12 +/- 0.03 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 18:07:13.64 -05:07:28.9: 12.88 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.33 +/- 0.01
Forced photometry filter KEPT candidate at 18:06:24.46 -04:10:50.3: ref_mag=12.33 +/- 0.01 new_mean_mag=11.1530 delta=1.17 (need > 0.90)
Forced photometry reference-image weighted average: 13.10 +/- 0.02
Forced photometry reference-image weighted average: 12.90 +/- 0.02
Forced photometry filter KEPT candidate at 17:57:30.07 -03:57:31.1: ref_mag=13.10 +/- 0.02 new_mean_mag=12.0416 delta=1.06 (need > 0.90)
Forced photometry filter KEPT candidate at 18:07:13.64 -05:07:28.9: ref_mag=12.90 +/- 0.02 new_mean_mag=11.7840 delta=1.11 (need > 0.90)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 18:03:39.14 -03:45:13.0: 13.76 +/- 0.05 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 18:03:39.14 -03:45:13.0: 13.74 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.75 +/- 0.03
Forced photometry filter KEPT candidate at 18:03:39.14 -03:45:13.0: ref_mag=13.75 +/- 0.03 new_mean_mag=12.2881 delta=1.46 (need > 0.90)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 17:52:01.09 -05:34:53.2: 13.20 +/- 0.03 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 17:52:01.09 -05:34:53.2: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.02
Forced photometry filter KEPT candidate at 17:52:01.09 -05:34:53.2: ref_mag=13.18 +/- 0.02 new_mean_mag=12.2054 delta=0.97 (need > 0.90)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 17:49:21.15 -05:12:27.5: 12.97 +/- 0.03 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 17:49:21.15 -05:12:27.5: 12.93 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.02
Forced photometry filter KEPT candidate at 17:49:21.15 -05:12:27.5: ref_mag=12.95 +/- 0.02 new_mean_mag=11.9518 delta=1.00 (need > 0.90)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 17:57:30.49 -04:05:39.9: 12.97 +/- 0.03 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 18:03:11.48 -04:15:12.6: 12.58 +/- 0.02 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 18:05:05.96 -04:10:39.2: 11.18 +/- 0.00 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 17:57:30.49 -04:05:39.9: 12.99 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.02
Forced photometry filter KEPT candidate at 17:57:30.49 -04:05:39.9: ref_mag=12.98 +/- 0.02 new_mean_mag=12.0366 delta=0.94 (need > 0.90)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 18:03:11.48 -04:15:12.6: 12.57 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.58 +/- 0.01
Forced photometry filter KEPT candidate at 18:03:11.48 -04:15:12.6: ref_mag=12.58 +/- 0.01 new_mean_mag=11.1546 delta=1.42 (need > 0.90)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 18:05:05.96 -04:10:39.2: 11.21 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.20 +/- 0.00
Forced photometry filter KEPT candidate at 18:05:05.96 -04:10:39.2: ref_mag=11.20 +/- 0.00 new_mean_mag=10.1279 delta=1.07 (need > 0.90)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 18:06:30.59 -04:21:59.1: 12.59 +/- 0.02 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 18:03:52.10 -03:49:56.7: 13.43 +/- 0.04 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 18:06:30.59 -04:21:59.1: 12.59 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.59 +/- 0.01
Forced photometry filter KEPT candidate at 18:06:30.59 -04:21:59.1: ref_mag=12.59 +/- 0.01 new_mean_mag=11.5180 delta=1.07 (need > 0.90)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 18:03:52.10 -03:49:56.7: 13.44 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.03
Forced photometry filter KEPT candidate at 18:03:52.10 -03:49:56.7: ref_mag=13.44 +/- 0.03 new_mean_mag=11.9679 delta=1.47 (need > 0.90)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 17:49:40.32 -05:06:09.9: 12.91 +/- 0.03 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 17:49:40.32 -05:06:09.9: 12.94 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.02
Forced photometry filter KEPT candidate at 17:49:40.32 -05:06:09.9: ref_mag=12.92 +/- 0.02 new_mean_mag=11.8638 delta=1.06 (need > 0.90)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 18:07:16.51 -04:55:49.2: 12.54 +/- 0.02 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 18:07:16.51 -04:55:49.2: 12.58 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.56 +/- 0.01
Forced photometry filter KEPT candidate at 18:07:16.51 -04:55:49.2: ref_mag=12.56 +/- 0.01 new_mean_mag=11.4429 delta=1.12 (need > 0.90)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 17:51:45.65 -05:00:36.6: 13.25 +/- 0.04 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 17:51:45.65 -05:00:36.6: 13.25 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.25 +/- 0.03
Forced photometry filter KEPT candidate at 17:51:45.65 -05:00:36.6: ref_mag=13.25 +/- 0.03 new_mean_mag=12.2383 delta=1.01 (need > 0.90)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 17:49:56.07 -03:38:25.6: 13.25 +/- 0.03 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 17:49:20.81 -04:42:55.0: 13.21 +/- 0.03 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 17:49:56.07 -03:38:25.6: 13.34 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.03
Forced photometry filter KEPT candidate at 17:49:56.07 -03:38:25.6: ref_mag=13.29 +/- 0.03 new_mean_mag=11.9696 delta=1.32 (need > 0.90)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 17:49:20.81 -04:42:55.0: 13.21 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Forced photometry filter KEPT candidate at 17:49:20.81 -04:42:55.0: ref_mag=13.21 +/- 0.02 new_mean_mag=12.1903 delta=1.02 (need > 0.90)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 18:04:49.07 -04:19:33.8: 10.72 +/- 0.00 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 18:04:49.07 -04:19:33.8: 10.74 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.73 +/- 0.00
Forced photometry filter KEPT candidate at 18:04:49.07 -04:19:33.8: ref_mag=10.73 +/- 0.00 new_mean_mag=9.6688 delta=1.06 (need > 0.90)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 17:50:01.66 -05:16:03.9: 13.38 +/- 0.04 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 17:50:01.66 -05:16:03.9: 13.37 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.03
Forced photometry filter KEPT candidate at 17:50:01.66 -05:16:03.9: ref_mag=13.38 +/- 0.03 new_mean_mag=12.0665 delta=1.31 (need > 0.90)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 17:49:47.90 -05:14:01.6: 13.59 +/- 0.05 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 17:49:47.90 -05:14:01.6: 13.58 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.04
Forced photometry filter KEPT candidate at 17:49:47.90 -05:14:01.6: ref_mag=13.59 +/- 0.04 new_mean_mag=12.3837 delta=1.20 (need > 0.90)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 17:51:56.01 -05:28:59.2: 12.50 +/- 0.02 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 17:51:56.01 -05:28:59.2: 12.49 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.49 +/- 0.01
Forced photometry filter KEPT candidate at 17:51:56.01 -05:28:59.2: ref_mag=12.49 +/- 0.01 new_mean_mag=11.2982 delta=1.20 (need > 0.90)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 18:03:05.60 -03:37:32.6: 11.94 +/- 0.01 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 18:03:05.60 -03:37:32.6: 11.98 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.96 +/- 0.01
Forced photometry filter KEPT candidate at 18:03:05.60 -03:37:32.6: ref_mag=11.96 +/- 0.01 new_mean_mag=10.9839 delta=0.98 (need > 0.90)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 17:57:36.71 -04:06:20.3: 11.94 +/- 0.01 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 18:06:36.82 -04:58:13.0: 11.91 +/- 0.01 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 18:01:52.77 -03:53:49.4: 13.18 +/- 0.03 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 17:57:36.71 -04:06:20.3: 11.95 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.95 +/- 0.01
Forced photometry filter KEPT candidate at 17:57:36.71 -04:06:20.3: ref_mag=11.95 +/- 0.01 new_mean_mag=10.9607 delta=0.99 (need > 0.90)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 18:06:36.82 -04:58:13.0: 11.90 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.91 +/- 0.01
Forced photometry filter KEPT candidate at 18:06:36.82 -04:58:13.0: ref_mag=11.91 +/- 0.01 new_mean_mag=10.8935 delta=1.01 (need > 0.90)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 17:50:57.28 -06:07:31.6: 13.18 +/- 0.04 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 18:01:52.77 -03:53:49.4: 13.27 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.02
Forced photometry filter KEPT candidate at 18:01:52.77 -03:53:49.4: ref_mag=13.23 +/- 0.02 new_mean_mag=11.9607 delta=1.27 (need > 0.90)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 17:50:57.28 -06:07:31.6: 13.20 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.03
Forced photometry filter KEPT candidate at 17:50:57.28 -06:07:31.6: ref_mag=13.19 +/- 0.03 new_mean_mag=12.1008 delta=1.09 (need > 0.90)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 17:51:02.70 -06:05:04.9: 13.14 +/- 0.03 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 17:49:52.86 -05:15:34.9: 11.81 +/- 0.01 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 17:51:02.70 -06:05:04.9: 13.28 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.02
Forced photometry filter KEPT candidate at 17:51:02.70 -06:05:04.9: ref_mag=13.20 +/- 0.02 new_mean_mag=12.0757 delta=1.13 (need > 0.90)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 17:49:52.86 -05:15:34.9: 11.78 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.79 +/- 0.01
Forced photometry filter KEPT candidate at 17:49:52.86 -05:15:34.9: ref_mag=11.79 +/- 0.01 new_mean_mag=10.8802 delta=0.91 (need > 0.90)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 17:49:26.20 -05:07:05.6: 13.53 +/- 0.04 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 17:49:26.20 -05:07:05.6: 13.54 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.54 +/- 0.03
Forced photometry filter KEPT candidate at 17:49:26.20 -05:07:05.6: ref_mag=13.54 +/- 0.03 new_mean_mag=12.3803 delta=1.16 (need > 0.90)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 17:56:44.38 -03:52:15.4: 13.55 +/- 0.04 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 18:04:07.13 -03:39:39.4: 14.01 +/- 0.06 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 17:56:44.38 -03:52:15.4: 13.58 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.03
Forced photometry filter KEPT candidate at 17:56:44.38 -03:52:15.4: ref_mag=13.56 +/- 0.03 new_mean_mag=12.3330 delta=1.23 (need > 0.90)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 18:04:07.13 -03:39:39.4: 14.06 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.04 +/- 0.04
Forced photometry filter KEPT candidate at 18:04:07.13 -03:39:39.4: ref_mag=14.04 +/- 0.04 new_mean_mag=12.5503 delta=1.49 (need > 0.90)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 18:03:46.30 -03:47:21.9: 13.12 +/- 0.03 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 18:03:46.30 -03:47:21.9: 13.08 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.02
Forced photometry filter KEPT candidate at 18:03:46.30 -03:47:21.9: ref_mag=13.10 +/- 0.02 new_mean_mag=11.7761 delta=1.32 (need > 0.90)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 18:03:02.40 -03:37:43.0: 13.13 +/- 0.03 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 18:03:02.40 -03:37:43.0: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Forced photometry filter KEPT candidate at 18:03:02.40 -03:37:43.0: ref_mag=13.14 +/- 0.02 new_mean_mag=12.0264 delta=1.12 (need > 0.90)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 17:52:10.70 -05:10:57.0: 13.11 +/- 0.03 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 17:52:10.70 -05:10:57.0: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Forced photometry filter KEPT candidate at 17:52:10.70 -05:10:57.0: ref_mag=13.14 +/- 0.02 new_mean_mag=11.8002 delta=1.34 (need > 0.90)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 17:48:26.50 -04:48:54.5: 13.12 +/- 0.03 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 17:48:26.50 -04:48:54.5: 13.17 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.02
Forced photometry filter KEPT candidate at 17:48:26.50 -04:48:54.5: ref_mag=13.15 +/- 0.02 new_mean_mag=12.0461 delta=1.10 (need > 0.90)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 17:48:57.12 -04:46:05.6: 13.11 +/- 0.03 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 17:48:57.12 -04:46:05.6: 13.09 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.02
Forced photometry filter KEPT candidate at 17:48:57.12 -04:46:05.6: ref_mag=13.10 +/- 0.02 new_mean_mag=12.0903 delta=1.01 (need > 0.90)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 18:04:01.91 -04:01:58.3: 11.72 +/- 0.01 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 18:04:01.91 -04:01:58.3: 11.74 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.73 +/- 0.01
Forced photometry filter KEPT candidate at 18:04:01.91 -04:01:58.3: ref_mag=11.73 +/- 0.01 new_mean_mag=10.6490 delta=1.08 (need > 0.90)
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-09_01-46-03_20.00sec_4.90C_LIGHT_0086.fits at 18:06:14.50 -04:03:49.5: 11.71 +/- 0.01 detection
Forced photometry on wcs_Ser-07-Q2b1x1_2026-06-12_02-15-36_20.00sec_4.90C_LIGHT_0094.fits at 18:06:14.50 -04:03:49.5: 11.67 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.69 +/- 0.01
Forced photometry filter KEPT candidate at 18:06:14.50 -04:03:49.5: ref_mag=11.69 +/- 0.01 new_mean_mag=10.7040 delta=0.98 (need > 0.90)
Adding exclusion_list_local.txt__out06631.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06907.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10122.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10330.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10550.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11799.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12032.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12034.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12101.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12106.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12377.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12463.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12496.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12605.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12881.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13094.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13170.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13786.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13806.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14144.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14544.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14972.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15242.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15551.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17381.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17497.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17995.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out18350.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out18351.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out18752.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out18917.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out18984.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19169.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19535.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20036.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20212.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20422.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20660.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20763.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20890.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21436.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21581.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21611.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21645.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 57s
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: 23s
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Considering the candidate 12881_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
Preparing report for the candidate 12881_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
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Considering the candidate 11799_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
Preparing report for the candidate 11799_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
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Considering the candidate 19535_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
Preparing report for the candidate 19535_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
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Considering the candidate 12463_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
Preparing report for the candidate 12463_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
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Considering the candidate 20763_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
Preparing report for the candidate 20763_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
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Considering the candidate 10330_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
Preparing report for the candidate 10330_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
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Considering the candidate 12101_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
Preparing report for the candidate 12101_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
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Considering the candidate 14544_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
Preparing report for the candidate 14544_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
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Considering the candidate 12032_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
Preparing report for the candidate 12032_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
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Considering the candidate 18351_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
Preparing report for the candidate 18351_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
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Considering the candidate 20890_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
Preparing report for the candidate 20890_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
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Considering the candidate 10122_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
Preparing report for the candidate 10122_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
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Considering the candidate 12496_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
Preparing report for the candidate 12496_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
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Considering the candidate 18917_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
Preparing report for the candidate 18917_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
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Considering the candidate 17995_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
Preparing report for the candidate 17995_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
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Considering the candidate 18350_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
Preparing report for the candidate 18350_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
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Considering the candidate 13927_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
The candidate 13927_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336 did not pass the final checks
**** FOUND 18:06:37.83 -04:55:16.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 17381_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
Preparing report for the candidate 17381_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
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Considering the candidate 20422_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
Preparing report for the candidate 20422_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
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Considering the candidate 13568_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
The candidate 13568_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336 did not pass the final checks
**** FOUND 17:51:51.93 -05:01:17.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 13170_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
Preparing report for the candidate 13170_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
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Considering the candidate 14144_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
Preparing report for the candidate 14144_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
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Considering the candidate 13786_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
Preparing report for the candidate 13786_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
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Considering the candidate 21581_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
Preparing report for the candidate 21581_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
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Considering the candidate 15551_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
Preparing report for the candidate 15551_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
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Considering the candidate 17497_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
Preparing report for the candidate 17497_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
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Considering the candidate 12106_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
Preparing report for the candidate 12106_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
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Considering the candidate 12377_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
Preparing report for the candidate 12377_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
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Considering the candidate 14239_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
The candidate 14239_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336 did not pass the final checks
**** FOUND 17:49:51.05 -04:55:26.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 10550_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
Preparing report for the candidate 10550_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
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Considering the candidate 21611_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
Preparing report for the candidate 21611_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
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Considering the candidate 18752_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
Preparing report for the candidate 18752_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
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Considering the candidate 13806_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
Preparing report for the candidate 13806_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
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Considering the candidate 20036_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
Preparing report for the candidate 20036_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
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Considering the candidate 06631_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
Preparing report for the candidate 06631_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
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Considering the candidate 06907_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
Preparing report for the candidate 06907_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
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Considering the candidate 12034_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
Preparing report for the candidate 12034_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
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Considering the candidate 13094_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
Preparing report for the candidate 13094_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
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Considering the candidate 20212_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
Preparing report for the candidate 20212_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
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Considering the candidate 21436_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
Preparing report for the candidate 21436_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
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Considering the candidate 20660_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
Preparing report for the candidate 20660_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
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Considering the candidate 21645_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
Preparing report for the candidate 21645_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
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Considering the candidate 12605_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
Preparing report for the candidate 12605_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
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Considering the candidate 14972_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
Preparing report for the candidate 14972_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
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Considering the candidate 15242_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
Preparing report for the candidate 15242_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
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Considering the candidate 19169_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
Preparing report for the candidate 19169_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
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Considering the candidate 18984_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
Preparing report for the candidate 18984_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
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Considering the candidate 14529_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336
The candidate 14529_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336 did not pass the final checks
**** FOUND 18:06:15.35 -04:45:02.1 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 4s
make_report_in_HTML.sh TOTAL: 84s
Prepared the HTML report for the field Ser-07-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
17:50:57.28 -06:07:31.6
17:51:02.70 -06:05:04.9
17:52:01.09 -05:34:53.2
17:50:42.72 -05:32:38.6
17:51:56.01 -05:28:59.2
17:51:01.41 -05:18:50.4
17:51:53.37 -05:17:18.0
17:49:52.86 -05:15:34.9
17:50:55.19 -05:16:44.8
17:50:01.66 -05:16:03.9
17:49:47.90 -05:14:01.6
17:50:17.15 -05:12:49.8
17:49:21.15 -05:12:27.5
17:52:10.70 -05:10:57.0
18:07:13.64 -05:07:28.9
17:49:26.20 -05:07:05.6
17:49:40.32 -05:06:09.9
17:51:45.65 -05:00:36.6
18:06:36.82 -04:58:13.0
18:07:16.51 -04:55:49.2
17:51:07.00 -04:52:49.7
17:48:26.50 -04:48:54.5
17:48:57.12 -04:46:05.6
17:49:20.81 -04:42:55.0
18:06:30.59 -04:21:59.1
18:04:49.07 -04:19:33.8
18:03:11.48 -04:15:12.6
18:05:05.96 -04:10:39.2
18:06:24.46 -04:10:50.3
17:57:36.71 -04:06:20.3
17:57:30.49 -04:05:39.9
18:06:14.50 -04:03:49.5
18:04:01.91 -04:01:58.3
17:57:30.07 -03:57:31.1
18:01:52.77 -03:53:49.4
17:56:44.38 -03:52:15.4
18:03:52.10 -03:49:56.7
18:03:46.30 -03:47:21.9
18:03:08.91 -03:46:06.1
18:03:39.14 -03:45:13.0
18:04:07.13 -03:39:39.4
17:49:56.07 -03:38:25.6
18:03:05.60 -03:37:32.6
18:03:02.40 -03:37:43.0
Source monitoring: measuring positions from /data_ssd/NMW-TexasTech/workdir/img_2026-07-18_CI_Ser-07-Q2b1x1_041149_TTUQ2b1x1_928637_e4bqkijR/monitoring_positions.txt
Read 5102 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 262.1525 to 277.8969 deg, Dec -7.2834 to +3.2884 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 262.1525 to 277.8969 deg, Dec -7.2834 to 3.2884 deg
Loaded 5331 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): 1886 out of 1923 total matches.
Matched with Tycho-2 1923 out of 5102 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits via Tycho-2
util/pixel_flux_airmass_correction processing wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits
Observation time (mid-exposure, UTC): JD 2461239.88235 (FITS header)
Observing site: lat= +33.748292 deg lon= -101.958319 deg east-positive (SITELAT/SITELONG FITS header keywords)
Frame center (pixel 4788.5 3194.5): RA= 270.00302 deg Dec= -2.00171 deg
Frame center: alt= +21.854 deg az= 254.664 deg airmass= 2.6644
Header cross-check: CENTALT= 22.092 deg (difference -0.238 deg)
Header cross-check: AIRMASS= 2.6432 (we compute 2.6644)
Airmass zero-point fit: REJECT_K_RANGE k= -0.1973 +/- 0.0414 mag/airmass N= 1621 airmass span 1.9394-4.3516 scatter 0.8468 mag
Source monitoring: airmass zero-point for wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits: REJECT_K_RANGE -0.531252 +0.197250 2.6644 -0.1973 1621 2.4122 0.8468 1.9394 4.3516
Forced photometry (list mode): image=wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits list=monitoring_pixlist2851794.tmp aperture=4.5
Image size: 9576 x 6388
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
Saturation level: 57000.0
Calibration (from calib.txt_param_monitoring, fit_function=3): cal_mag = 0.000000 * x^2 + 1.000000 * x + 20.109650
Forced photometry: center=(57.08, 5437.98) aperture=4.5
Annulus: inner=9.00 outer=22.50
Background annulus: 1341 pixels
Iterative clipping converged after 1 iterations, 1337/1341 pixels remain
SExtractor background: mode=1175.05 median=1177.00 mean=1178.30 sigma=75.59 -> bg=1175.05 (1337 pixels)
Aperture sum=19718.89 N_eff=15.9043
Net flux=1030.49 noise=301.44 SNR=3.42
Instrumental magnitude: -7.5326
Calibrated magnitude: 12.5770
Source monitoring: 1 position(s) measured on wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-10-24_20.00sec_5.00C_LIGHT_0335.fits (aperture 4.5 pix)
Read 4569 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 262.1636 to 277.9301 deg, Dec -7.2817 to +3.2870 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 262.1636 to 277.9301 deg, Dec -7.2817 to 3.2870 deg
Loaded 5328 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): 1529 out of 1559 total matches.
Matched with Tycho-2 1559 out of 4569 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits via Tycho-2
util/pixel_flux_airmass_correction processing wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits
Observation time (mid-exposure, UTC): JD 2461239.88284 (FITS header)
Observing site: lat= +33.748292 deg lon= -101.958319 deg east-positive (SITELAT/SITELONG FITS header keywords)
Frame center (pixel 4788.5 3194.5): RA= 270.01446 deg Dec= -1.99902 deg
Frame center: alt= +21.725 deg az= 254.760 deg airmass= 2.6793
Header cross-check: CENTALT= 21.954 deg (difference -0.229 deg)
Header cross-check: AIRMASS= 2.6587 (we compute 2.6793)
Airmass zero-point fit: REJECT_NOISY_FIT k= -0.7155 +/- 0.0504 mag/airmass N= 1334 airmass span 1.9435-4.3533 scatter 0.9029 mag
Source monitoring: airmass zero-point for wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits: REJECT_NOISY_FIT -1.974679 +0.715477 2.6793 -0.7155 1334 2.4099 0.9029 1.9435 4.3533
Forced photometry (list mode): image=wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits list=monitoring_pixlist2851794.tmp aperture=4.5
Image size: 9576 x 6388
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
Saturation level: 57000.0
Calibration (from calib.txt_param_monitoring, fit_function=3): cal_mag = 0.000000 * x^2 + 1.000000 * x + 19.976300
Forced photometry: center=(64.28, 5439.72) aperture=4.5
Annulus: inner=9.00 outer=22.50
Background annulus: 1339 pixels
Iterative clipping converged after 3 iterations, 1330/1339 pixels remain
SExtractor background: mode=1359.14 median=1356.00 mean=1353.91 sigma=81.48 -> bg=1359.14 (1330 pixels)
Aperture sum=21904.19 N_eff=15.9043
Net flux=288.00 noise=324.93 SNR=0.89
Instrumental magnitude: -7.4723
Calibrated magnitude: 12.5040
Source monitoring: 1 position(s) measured on wcs_fd_Ser-07-Q2b1x1_2026-07-18_04-11-07_20.00sec_5.00C_LIGHT_0336.fits (aperture 4.5 pix)
########### Completed Ser-07-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
18:07:13.64 -05:07:28.9
17:51:01.41 -05:18:50.4
17:57:30.07 -03:57:31.1
17:50:17.15 -05:12:49.8
18:03:08.91 -03:46:06.1
17:50:42.72 -05:32:38.6
17:50:55.19 -05:16:44.8
17:51:07.00 -04:52:49.7
17:51:53.37 -05:17:18.0
18:06:24.46 -04:10:50.3
18:03:39.14 -03:45:13.0
17:52:01.09 -05:34:53.2
17:49:21.15 -05:12:27.5
17:57:30.49 -04:05:39.9
18:03:11.48 -04:15:12.6
18:05:05.96 -04:10:39.2
18:06:30.59 -04:21:59.1
18:03:52.10 -03:49:56.7
17:49:40.32 -05:06:09.9
18:07:16.51 -04:55:49.2
17:51:45.65 -05:00:36.6
17:49:56.07 -03:38:25.6
17:49:20.81 -04:42:55.0
18:04:49.07 -04:19:33.8
17:50:01.66 -05:16:03.9
17:49:47.90 -05:14:01.6
17:51:56.01 -05:28:59.2
18:03:05.60 -03:37:32.6
17:57:36.71 -04:06:20.3
18:06:36.82 -04:58:13.0
18:01:52.77 -03:53:49.4
17:50:57.28 -06:07:31.6
17:51:02.70 -06:05:04.9
17:49:52.86 -05:15:34.9
17:49:26.20 -05:07:05.6
17:56:44.38 -03:52:15.4
18:04:07.13 -03:39:39.4
18:03:46.30 -03:47:21.9
18:03:02.40 -03:37:43.0
17:52:10.70 -05:10:57.0
17:48:26.50 -04:48:54.5
17:48:57.12 -04:46:05.6
18:04:01.91 -04:01:58.3
18:06:14.50 -04:03:49.5
###################################################################################
18:07:13.64 -05:07:28.9 -- not an asteroid (will add it to exclusion list)
17:51:01.41 -05:18:50.4 -- not an asteroid (will add it to exclusion list)
17:57:30.07 -03:57:31.1 -- not an asteroid (will add it to exclusion list)
17:50:17.15 -05:12:49.8 -- not an asteroid (will add it to exclusion list)
18:03:08.91 -03:46:06.1 -- not an asteroid (will add it to exclusion list)
17:50:42.72 -05:32:38.6 -- not an asteroid (will add it to exclusion list)
17:50:55.19 -05:16:44.8 -- not an asteroid (will add it to exclusion list)
17:51:07.00 -04:52:49.7 -- not an asteroid (will add it to exclusion list)
17:51:53.37 -05:17:18.0 -- not an asteroid (will add it to exclusion list)
18:06:24.46 -04:10:50.3 -- not an asteroid (will add it to exclusion list)
18:03:39.14 -03:45:13.0 -- not an asteroid (will add it to exclusion list)
17:52:01.09 -05:34:53.2 -- not an asteroid (will add it to exclusion list)
17:49:21.15 -05:12:27.5 -- not an asteroid (will add it to exclusion list)
17:57:30.49 -04:05:39.9 -- not an asteroid (will add it to exclusion list)
18:03:11.48 -04:15:12.6 -- not an asteroid (will add it to exclusion list)
18:05:05.96 -04:10:39.2 -- not an asteroid (will add it to exclusion list)
18:06:30.59 -04:21:59.1 -- not an asteroid (will add it to exclusion list)
18:03:52.10 -03:49:56.7 -- not an asteroid (will add it to exclusion list)
17:49:40.32 -05:06:09.9 -- not an asteroid (will add it to exclusion list)
18:07:16.51 -04:55:49.2 -- not an asteroid (will add it to exclusion list)
17:51:45.65 -05:00:36.6 -- not an asteroid (will add it to exclusion list)
17:49:56.07 -03:38:25.6 -- not an asteroid (will add it to exclusion list)
17:49:20.81 -04:42:55.0 -- not an asteroid (will add it to exclusion list)
18:04:49.07 -04:19:33.8 -- not an asteroid (will add it to exclusion list)
17:50:01.66 -05:16:03.9 -- not an asteroid (will add it to exclusion list)
17:49:47.90 -05:14:01.6 -- not an asteroid (will add it to exclusion list)
17:51:56.01 -05:28:59.2 -- not an asteroid (will add it to exclusion list)
18:03:05.60 -03:37:32.6 -- not an asteroid (will add it to exclusion list)
17:57:36.71 -04:06:20.3 -- not an asteroid (will add it to exclusion list)
18:06:36.82 -04:58:13.0 -- not an asteroid (will add it to exclusion list)
18:01:52.77 -03:53:49.4 -- not an asteroid (will add it to exclusion list)
17:50:57.28 -06:07:31.6 -- not an asteroid (will add it to exclusion list)
17:51:02.70 -06:05:04.9 -- not an asteroid (will add it to exclusion list)
17:49:52.86 -05:15:34.9 -- not an asteroid (will add it to exclusion list)
17:49:26.20 -05:07:05.6 -- not an asteroid (will add it to exclusion list)
17:56:44.38 -03:52:15.4 -- asteroid (will NOT add it to exclusion list)
18:04:07.13 -03:39:39.4 -- not an asteroid (will add it to exclusion list)
18:03:46.30 -03:47:21.9 -- not an asteroid (will add it to exclusion list)
18:03:02.40 -03:37:43.0 -- not an asteroid (will add it to exclusion list)
17:52:10.70 -05:10:57.0 -- not an asteroid (will add it to exclusion list)
17:48:26.50 -04:48:54.5 -- not an asteroid (will add it to exclusion list)
17:48:57.12 -04:46:05.6 -- not an asteroid (will add it to exclusion list)
18:04:01.91 -04:01:58.3 -- not an asteroid (will add it to exclusion list)
18:06:14.50 -04:03:49.5 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
17:48:26.50 -04:48:54.5 -- does not seem to be a hot pixel (will add it to exclusion list)
17:48:57.12 -04:46:05.6 -- does not seem to be a hot pixel (will add it to exclusion list)
17:49:20.81 -04:42:55.0 -- does not seem to be a hot pixel (will add it to exclusion list)
17:49:21.15 -05:12:27.5 -- does not seem to be a hot pixel (will add it to exclusion list)
17:49:26.20 -05:07:05.6 -- does not seem to be a hot pixel (will add it to exclusion list)
17:49:40.32 -05:06:09.9 -- does not seem to be a hot pixel (will add it to exclusion list)
17:49:47.90 -05:14:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
17:49:52.86 -05:15:34.9 -- does not seem to be a hot pixel (will add it to exclusion list)
17:49:56.07 -03:38:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
17:50:01.66 -05:16:03.9 -- does not seem to be a hot pixel (will add it to exclusion list)
17:50:17.15 -05:12:49.8 -- does not seem to be a hot pixel (will add it to exclusion list)
17:50:42.72 -05:32:38.6 -- does not seem to be a hot pixel (will add it to exclusion list)
17:50:55.19 -05:16:44.8 -- does not seem to be a hot pixel (will add it to exclusion list)
17:50:57.28 -06:07:31.6 -- does not seem to be a hot pixel (will add it to exclusion list)
17:51:01.41 -05:18:50.4 -- does not seem to be a hot pixel (will add it to exclusion list)
17:51:02.70 -06:05:04.9 -- does not seem to be a hot pixel (will add it to exclusion list)
17:51:07.00 -04:52:49.7 -- does not seem to be a hot pixel (will add it to exclusion list)
17:51:45.65 -05:00:36.6 -- does not seem to be a hot pixel (will add it to exclusion list)
17:51:53.37 -05:17:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
17:51:56.01 -05:28:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
17:52:01.09 -05:34:53.2 -- does not seem to be a hot pixel (will add it to exclusion list)
17:52:10.70 -05:10:57.0 -- does not seem to be a hot pixel (will add it to exclusion list)
17:57:30.07 -03:57:31.1 -- does not seem to be a hot pixel (will add it to exclusion list)
17:57:30.49 -04:05:39.9 -- does not seem to be a hot pixel (will add it to exclusion list)
17:57:36.71 -04:06:20.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:01:52.77 -03:53:49.4 -- does not seem to be a hot pixel (will add it to exclusion list)
18:03:02.40 -03:37:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:03:05.60 -03:37:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:03:08.91 -03:46:06.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:03:11.48 -04:15:12.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:03:39.14 -03:45:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:03:46.30 -03:47:21.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:03:52.10 -03:49:56.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:04:01.91 -04:01:58.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:04:07.13 -03:39:39.4 -- does not seem to be a hot pixel (will add it to exclusion list)
18:04:49.07 -04:19:33.8 -- does not seem to be a hot pixel (will add it to exclusion list)
18:05:05.96 -04:10:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:06:14.50 -04:03:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:06:24.46 -04:10:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:06:30.59 -04:21:59.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:06:36.82 -04:58:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:07:13.64 -05:07:28.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:07:16.51 -04:55:49.2 -- 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)
17:48:26.50 -04:48:54.5 -- not a known variable star
17:48:57.12 -04:46:05.6 -- a known variable star
17:49:20.81 -04:42:55.0 -- a known variable star
17:49:21.15 -05:12:27.5 -- not a known variable star
17:49:26.20 -05:07:05.6 -- not a known variable star
17:49:40.32 -05:06:09.9 -- a known variable star
17:49:47.90 -05:14:01.6 -- not a known variable star
17:49:52.86 -05:15:34.9 -- not a known variable star
17:49:56.07 -03:38:25.6 -- a known variable star
17:50:01.66 -05:16:03.9 -- not a known variable star
17:50:17.15 -05:12:49.8 -- a known variable star
17:50:42.72 -05:32:38.6 -- not a known variable star
17:50:55.19 -05:16:44.8 -- not a known variable star
17:50:57.28 -06:07:31.6 -- not a known variable star
17:51:01.41 -05:18:50.4 -- not a known variable star
17:51:02.70 -06:05:04.9 -- a known variable star
17:51:07.00 -04:52:49.7 -- not a known variable star
17:51:45.65 -05:00:36.6 -- not a known variable star
17:51:53.37 -05:17:18.0 -- not a known variable star
17:51:56.01 -05:28:59.2 -- a known variable star
17:52:01.09 -05:34:53.2 -- not a known variable star
17:52:10.70 -05:10:57.0 -- a known variable star
17:57:30.07 -03:57:31.1 -- a known variable star
17:57:30.49 -04:05:39.9 -- not a known variable star
17:57:36.71 -04:06:20.3 -- a known variable star
18:01:52.77 -03:53:49.4 -- not a known variable star
18:03:02.40 -03:37:43.0 -- not a known variable star
18:03:05.60 -03:37:32.6 -- a known variable star
18:03:08.91 -03:46:06.1 -- not a known variable star
18:03:11.48 -04:15:12.6 -- not a known variable star
18:03:39.14 -03:45:13.0 -- not a known variable star
18:03:46.30 -03:47:21.9 -- not a known variable star
18:03:52.10 -03:49:56.7 -- not a known variable star
18:04:01.91 -04:01:58.3 -- not a known variable star
18:04:07.13 -03:39:39.4 -- not a known variable star
18:04:49.07 -04:19:33.8 -- not a known variable star
18:05:05.96 -04:10:39.2 -- a known variable star
18:06:14.50 -04:03:49.5 -- not a known variable star
18:06:24.46 -04:10:50.3 -- not a known variable star
18:06:30.59 -04:21:59.1 -- not a known variable star
18:06:36.82 -04:58:13.0 -- a known variable star
18:07:13.64 -05:07:28.9 -- not a known variable star
18:07:16.51 -04:55:49.2 -- not a known variable star
Found 30 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
43 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 43 (excluding asteroids and hot pixels, 30 new), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461239.88234881 -observatory V36
07:12:21.92 +17:31:51.1 Mercury (4.0mag)
10:44:32.30 +09:02:25.4 Venus (-4.2mag)
04:47:58.85 +22:19:00.2 Mars (1.3mag)
08:23:59.56 +19:47:51.4 Jupiter (-1.8mag)
00:56:32.00 +03:22:20.3 Saturn (0.7mag)
04:08:42.11 +20:48:59.7 Uranus (5.8mag)
00:16:55.51 +00:19:35.0 Neptune (7.7mag)
20:30:09.68 -23:21:32.4 Pluto (14.4mag)
11:14:33.00 +02:23:35.8 Moon (-9.4mag)
-rw-r--r-- 1 apache apache 361 Jul 18 08:29 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461239.88234881:
08:23:55.07 +19:48:09.0 Io (6.0mag)
08:24:10.75 +19:47:08.4 Europa (6.3mag)
08:24:15.13 +19:46:49.7 Ganymede (5.6mag)
08:23:33.78 +19:49:31.6 Callisto (6.8mag)
08:22:10.09 +19:35:37.8 Himalia (15.7mag)
08:23:57.74 +19:47:59.5 Thebe (16.6mag)
08:21:31.13 +19:38:20.4 Elara (17.7mag)
08:27:45.53 +19:37:45.5 Pasiphae (17.9mag)
08:28:29.35 +19:54:09.7 Carme (19.0mag)
00:56:41.96 +03:22:28.9 Titan (8.5mag)
00:56:30.86 +03:22:31.0 Rhea (9.8mag)
00:55:57.53 +03:20:09.9 Iapetus (11.2mag)
00:56:19.03 +03:22:10.1 Hyperion (14.5mag)
00:56:21.97 +03:18:24.1 Phoebe (16.5mag)
-rw-r--r-- 1 apache apache 568 Jul 18 08:29 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461239.88234881:
17:58:38.73 -31:00:53.5 JWST
16:28:31.94 +46:34:24.4 Chandra
05:15:34.82 +44:39:53.6 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jul 18 08:29 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461239.88234881 -observatory V36
02:47:28.84 +15:21:09.5 17.8mag P/1996 R2 (Lagerkvist)
18:12:04.62 -34:32:41.9 13.8mag P/2010 H2 (Vales)
06:33:41.03 -68:17:15.5 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:03:32.73 +32:35:12.9 17.6mag C/2017 K2 (PANSTARRS)
02:28:40.70 +21:24:09.8 15.8mag P/2021 N1 (ZTF)
22:54:26.25 +32:13:23.5 17.3mag C/2022 E2 (ATLAS)
06:21:27.68 +26:50:44.6 16.7mag C/2022 N2 (PANSTARRS)
10:02:35.09 +29:25:08.0 16.9mag C/2022 QE78 (ATLAS)
09:14:57.87 +05:08:05.0 17.9mag C/2022 R6 (PANSTARRS)
15:11:02.52 -11:35:17.3 17.8mag P/2023 B1 (PANSTARRS)
21:39:07.39 +67:28:51.5 17.9mag C/2023 H5 (Lemmon)
16:15:59.81 -10:54:29.1 14.0mag C/2023 R1 (PANSTARRS)
08:14:49.59 +66:09:21.0 17.9mag C/2024 A1 (ATLAS)
07:43:10.79 +30:23:59.7 14.8mag C/2024 E1 (Wierzchos)
15:12:45.56 +15:30:08.3 17.6mag C/2024 G6 (ATLAS)
19:30:50.49 +40:49:59.4 13.7mag C/2024 J3 (ATLAS)
21:38:45.09 +47:08:50.9 17.8mag C/2024 R4 (PANSTARRS)
04:57:07.72 -13:27:53.6 15.7mag C/2024 T5 (ATLAS)
06:41:06.11 +27:43:38.7 18.0mag C/2025 J1 (Borisov)
07:19:43.95 -13:38:47.5 16.9mag C/2025 R3 (PANSTARRS)
10:05:38.23 +22:04:20.4 17.5mag C/2025 V2 (Rankin)
12:47:34.40 +03:34:08.6 17.0mag C/2025 Y1 (ATLAS)
16:30:46.96 +79:07:35.8 17.2mag C/2026 A2 (Bok)
02:54:12.76 +45:34:12.0 16.8mag C/2026 B2 (Sun-Gao)
11:30:50.86 +05:52:57.5 17.0mag A/2026 E1
21:31:18.19 -18:09:47.4 7.1mag 10P/Tempel
11:17:21.99 -02:15:00.4 16.2mag 29P/Schwassmann-Wachmann
04:11:37.01 +30:24:35.3 17.9mag 47P/Ashbrook-Jackson
10:24:48.91 +11:26:12.4 17.1mag 63P/Wild
00:51:25.65 -05:02:48.5 15.5mag 65P/Gunn
04:46:45.20 +20:31:49.5 13.7mag 78P/Gehrels
02:34:50.34 +11:39:32.0 16.4mag 88P/Howell
06:59:07.45 +29:58:26.5 15.8mag 93P/Lovas
04:47:16.36 +31:19:52.4 16.7mag 114P/Wiseman-Skiff
08:28:18.43 +29:45:07.8 15.2mag 123P/West-Hartley
11:03:13.27 -02:03:52.7 16.9mag 124P/Mrkos
05:04:33.66 +21:00:45.8 16.2mag 128P/Shoemaker-Holt
05:51:17.58 +19:36:40.4 17.8mag 131P/Mueller
07:42:07.10 +15:13:55.4 16.5mag 141P-D/Machholz
03:20:20.17 -20:44:36.6 15.1mag 161P/Hartley-IRAS
06:02:02.94 +35:30:58.1 15.5mag 162P/SidingSpring
18:38:50.34 +20:35:58.6 14.0mag 169P/NEAT
01:59:50.11 +08:25:04.0 17.6mag 220P/McNaught
16:35:32.77 -08:44:58.3 17.2mag 235P/LINEAR
09:02:04.68 +32:31:49.5 18.0mag 240P/NEAT
20:37:51.99 -51:09:47.4 17.8mag 259P/Garradd
02:21:56.32 +15:50:40.3 15.6mag 260P/McNaught
06:01:42.23 +37:23:33.0 17.3mag 295P/LINEAR
15:06:33.76 +05:18:50.5 17.6mag 391P/Kowalski
08:41:51.29 +19:20:29.4 17.9mag 450P/LONEOS
08:04:18.31 +38:32:33.3 18.0mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.5K Jul 18 08:29 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
04:50:01.03 -02:22:33.80 ASASSN-26ej 2026-07-16.17 17.02
18:34:55.28 -31:41:00.90 ASASSN-26ek 2026-07-16.24 15.73
17:07:43.61 -44:21:53.50 ASASSN-26el 2026-07-15.86 16.01
14:45:08.35 +24:13:12.30 ASASSN-26ei 2026-07-16.17 16.46
10:00:46.44 -32:36:31.10 AT 2023mhb 2026-07-14.73 16.67
14:39:37.45 -11:22:36.20 AT 2026unl 2026-07-15.27 17.11
10:49:42.57 -11:25:55.80 ASASSN-26eh 2026-07-14.72 16.58
19:33:53.06 -07:15:00.80 ASASSN-26eg 2026-07-14.15 15.5
02:45:40.52 -27:55:30.30 ASASSN-26ef 2026-07-12.35 15.86
23:26:43.80 +04:42:39.70 SN 2026qtn 2026-07-12.22 16.47
02:19:17.26 +28:57:15.40 ASASSN-26ec 2026-07-11.53 2.78
18:31:15.56 -05:34:31.50 AT2026stb 2026-07-11.28 -1.29
13:36:08.24 +23:29:05.00 AT2026pjf 2026-07-10.18 -0.72
17:33:39.82 +04:22:36.70 SN2026pir 2026-07-9.86 -0.66
11:21:41.26 -50:33:36.30 ASASSN-26ed 2026-07-8.8 -1.3
23:41:42.11 +26:29:49.10 AT2026qil 2026-07-9.3 16.15
20:21:30.50 -32:03:40.10 ASASSN-26ee 2026-07-7.22 15.53
19:37:44.09 -05:35:42.80 AT2026ryu 2026-07-7.17 14.88
11:06:55.46 -04:07:04.50 AT2026qqg 2026-07-5.01 16.82
19:07:23.69 -74:13:37.30 AT2026qly 2026-07-5.02 17.31
17:57:43.80 +27:18:40.10 ASASSN-26ea 2026-07-5.07 16.67
19:59:01.43 -32:07:34.30 ASASSN-26eb 2026-07-4.97 15.52
18:46:50.35 -57:44:13.20 SN 2026qqp 2026-07-5.03 -0.92
19:17:31.69 -39:55:29.90 ASASSN-26dz 2026-07-5.14 15.91
19:14:31.37 +12:03:52.90 AT 2026rdg 2026-07-3.43 11.81
04:05:50.09 -70:24:34.40 AT 2026qpr 2026-06-30.4 15.96
13:45:37.49 -05:59:35.80 SN 2026pub 2026-06-30.09 16.01
16:41:15.63 +39:17:14.70 SN 2026pel 2026-06-26.38 16.07
10:14:40.19 -35:38:21.30 ASASSN-26dy 2026-06-25.99 15.63
14:47:21.56 -40:15:51.30 ASASSN-26dv 2026-06-23.03 14.62
13:38:49.79 -77:21:06.70 ASASSN-26dw 2026-06-23.04 16.09
00:59:27.90 +33:08:13.20 SN 2026mke 2026-06-22.39 17.13
11:10:44.73 -30:20:45.50 SN 2026nmv 2026-06-22.06 16.56
21:36:15.68 -21:19:12.50 AT2026oxh 2026-06-22.15 17.14
17:31:38.38 -56:05:51.90 ASASSN-26dx 2026-06-22.02 14.72
14:10:13.44 -38:46:46.10 AT2026pvk 2026-06-22.06 16.53
20:56:47.23 -18:31:05.20 AT2026plb 2026-06-21.31 16.4
15:44:29.68 +21:00:59.30 SN2026ore 2026-06-21.29 17.57
23:50:05.98 -14:01:41.30 AT2026oxl 2026-06-21.52 17.64
17:36:54.73 -18:10:04.20 AT2026ouj 2026-06-20.92 15.15
00:34:04.08 -30:22:09.20 AT2026ntk 2026-06-18.09 17.34
20:49:13.39 +25:17:59.20 ASASSN-26du 2026-06-15.39 15.93
23:09:30.84 +32:40:42.00 SN2026oxc 2026-06-14.35 16.83
02:02:26.78 +32:04:21.30 AT2026ovz 2026-06-14.59 15.39
21:26:28.11 -72:31:19.50 AT2026nwc 2026-06-11 17.05
17:54:57.33 +26:32:34.20 SN 2026odc 2026-06-11.23 17.62
13:55:59.94 +17:30:37.20 SN 2026nyq 2026-06-11.1 16.24
00:50:45.14 -71:38:36.90 ASASSN-26dt 2026-06-11.13 10.22
14:42:19.73 +19:11:35.60 SN2026nyp 2026-06-10.3 16.32
12:23:23.92 +12:56:43.50 SN2026mta 2026-06-8.29 16.69
12:30:18.51 +47:12:33.20 SN2026oao 2026-06-9.32 17.02
10:51:05.21 -42:28:56.60 AT2026nvf 2026-06-8.12 16.75
13:50:22.48 -07:35:00.00 SN2026npn 2026-06-8.02 17.58
00:56:07.17 +43:01:43.20 ASASSN-26dq 2026-06-7.43 13.58
01:07:49.46 +41:59:43.70 SN 2026obc 2026-06-7.43 15.15
21:11:25.22 +14:14:31.90 ASASSN-26dr 2026-06-7.24 16.24
06:21:27.06 -65:16:42.00 ASASSN-26ds 2026-06-2.97 15.02
20:07:38.15 -21:07:05.40 SN2026mho 2026-05-25.18 -1.12
11:29:42.55 +79:01:03.10 AT2026min 2026-05-24.21 16.63
11:44:32.95 -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
14:23:56.72 -58:37:47.60 ASASSN-26dn 2026-05-20.01 14.64
11:24:54.06 +47:57:01.60 AT2026nma 2026-05-20.29 15.46
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
15:16:06.61 -79:16:32.40 ASASSN-26dm 2026-05-19.03 14.44
11:24:25.21 -59:23:19.10 ASASSN-26dl 2026-05-18.02 13.55
13:45:51.52 -53:16:01.00 ASASSN-26dk 2026-05-18.16 12.96
02:05:49.69 -30:29:09.60 ASASSN-26dh 2026-05-18.43 15.37
17:50:22.87 -39:42:33.90 ASASSN-26dj 2026-05-17.05 15.7
01:13:11.60 -33:25:16.10 ASASSN-26dg 2026-05-13.41 16.8
16:44:31.77 -27:15:18.40 AT2026mhn 2026-05-12.33 15.8
09:46:31.08 -33:41:51.00 ASASSN-26di 2026-05-12.14 14.63
21:23:11.57 -19:09:45.00 AT2026kwu 2026-05-12.26 16.9
14:20:14.30 -30:20:51.90 AT2026ktm 2026-05-12.06 17.21
14:41:39.01 -37:13:46.40 AT2026lkm 2026-05-11.18 16.89
12:59:50.45 -10:58:38.80 SN2026kep 2026-05-9.06 17.5
13:37:29.61 -29:50:30.90 AT2026lkd 2026-05-9.09 17.23
09:46:42.01 -14:52:03.60 SN2026kmo 2026-05-8.99 17.51
15:03:05.28 +22:02:03.80 AT2026lxf 2026-05-8.34 13.72
10:23:49.41 -20:57:25.30 ASASSN-26df 2026-05-8.21 16.52
22:14:40.56 +05:04:51.60 2026lda 2026-05-7.56 16.2
21:35:33.81 -14:05:16.30 ASASSN-26de 2026-05-6.29 14.51
16:21:49.13 -61:36:14.60 ASASSN-26dd 2026-05-5.15 15.93
14:26:40.22 -24:48:37.50 AT2026lig 2026-05-4.27 14.63
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
04:50:01.03 -02:22:33.80 2026-07-16.17 17.02
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
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
09:55:21.28 +69:02:52.6 PNV J09552128+6902526 2026-06-13.933 18.9mag
19:51:21.42 +37:06:40.0 TCP J19512142+3706400 2026-06-17.2942 16.8mag
19:57:03.87 +37:41:46.4 TCP J19570387+3741464 2026-06-18.2638 17.5mag
00:42:32.04 +41:10:28.3 PNV J00423204+4110283 2026-06-26.059 16.6mag
02:19:17.36 +28:57:15.8 TCP J02191736+2857158 2026-07-12.3549 12.5mag
00:44:56.43 +41:57:41.6 PNV J00445643+4157416 2026-07-13.8026 17.98Cmag
-rw-r--r-- 1 apache apache 189K Jul 18 08:29 tocp_transients_list.txt
############################################################
Truncated list of recent TNS transients from https://www.wis-tns.org/ :
21:40:11.159 -09:00:57.92 AT 2026swa 2026-06-27.33 23.1049
21:35:24.753 -14:51:35.01 AT 2026svz 2026-06-27.33 22.2271
20:31:55.032 -25:17:26.05 AT 2026svy 2026-06-27.32 22.425
23:12:03.386 -07:08:51.16 AT 2026svx 2026-06-27.43 22.3341
21:38:52.469 -09:12:08.16 AT 2026svw 2026-06-27.33 20.826
21:24:07.399 -08:10:48.32 AT 2026svv 2026-06-27.34 22.9964
20:42:22.608 -20:56:09.99 AT 2026svu 2026-06-27.32 22.8033
22:49:29.419 -09:52:21.90 AT 2026svt 2026-06-27.41 23.2399
23:08:56.975 -10:56:50.31 AT 2026svs 2026-06-27.42 23.0562
23:03:48.038 -10:42:20.17 AT 2026svr 2026-06-27.42 23.1156
21:05:20.116 -12:39:02.09 AT 2026svq 2026-06-27.30 22.4649
04:03:37.997 -49:14:19.96 AT 2026svp 2026-06-26.43 23.1019
21:42:26.450 -12:30:39.78 AT 2026svo 2026-06-26.41 23.1202
22:23:57.549 -05:26:28.43 AT 2026svn 2026-06-26.40 23.0846
21:59:30.646 -08:36:23.43 AT 2026svm 2026-06-26.41 23.0458
00:40:45.913 -42:36:08.06 AT 2026svl 2026-06-26.42 23.627
22:01:49.708 -02:28:35.92 AT 2026svk 2026-06-26.41 22.3804
22:26:37.642 -04:12:59.57 AT 2026svj 2026-06-26.40 22.8575
21:46:45.471 -13:57:34.56 AT 2026svi 2026-06-26.41 22.7499
21:42:08.217 -14:29:27.43 AT 2026svh 2026-06-26.41 23.2705
-rw-r--r-- 1 apache apache 89K Jul 18 08:29 tns_transients_list.txt
