This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q1b1x1_034543_TTUQ1b1x1_1395907_ABJhZHwf
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 11 03.4061 2461347.9061 10.26 08:18:45.59 -31:51:11.9
250.82705 2.31928 galactic Pup Second-epoch detections are separated by 0.3" and 5.6 pix
The object was found in VSX 1" V0548 Pup
Type: SR:
# Max. Min./Amp. JD0 Period
11.700 V 12.800 V 2452914.40000 158.400000000000 M7
The object was not found in astcheck.
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:18:45.59 -31:51:11.9: 11.35 +/- 0.02 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:18:45.59 -31:51:11.9: 11.31 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.33 +/- 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 Lite
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
V0548 Pup,2461347.9061,10.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0548 Pup 20261103.4061 10.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 03.4061 2461347.9061 7.86 08:23:04.30 -38:48:29.5
257.05242 -0.90600 galactic Pup Second-epoch detections are separated by 1.0" and 4.9 pix
The object was found in VSX 2" ASAS J082304-3848.5
Type: MISC
# Max. Min./Amp. JD0 Period
9.530 V Y 0.800 V 2452750.10000 272.000000000000 M7
The object was not found in astcheck.
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:23:04.30 -38:48:29.5: 8.79 +/- 0.00 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:23:04.30 -38:48:29.5: 8.79 +/- 0.00 detection
Forced photometry reference-image weighted average: 8.79 +/- 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 Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J082304-3848.5,2461347.9061,7.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J082304-3848.5 20261103.4061 7.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 03.4061 2461347.9061 12.97 08:18:37.68 -33:38:10.7
252.28617 1.29312 galactic Pup Second-epoch detections are separated by 2.7" and 5.8 pix
The object was found in VSX 4" GDS_J0818375-333814
Type: VAR
# Max. Min./Amp. JD0 Period
13.510 r Y 0.710 r
The object was not found in astcheck.
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:18:37.68 -33:38:10.7: 14.26 +/- 0.21 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:18:37.68 -33:38:10.7: 14.44 +/- 0.25 detection
Forced photometry reference-image weighted average: 14.34 +/- 0.16
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 Lite
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
GDS_J0818375-333814,2461347.9061,12.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J0818375-333814 20261103.4061 12.97CV 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 11 03.4061 2461347.9061 12.70 08:24:42.77 -32:26:53.0
252.03396 3.01775 galactic Pup Second-epoch detections are separated by 1.3" and 5.8 pix
The object was found in VSX 1" GDS_J0824428-322651
Type: M
# Max. Min./Amp. JD0 Period
15.660 r Y 3.030 r 329.100000000000 M6
The object was not found in astcheck.
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:24:42.77 -32:26:53.0: 14.85 +/- 0.34 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:24:42.77 -32:26:53.0: 14.88 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.85 +/- 0.34
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 Lite
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
GDS_J0824428-322651,2461347.9061,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J0824428-322651 20261103.4061 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 03.4061 2461347.9061 13.01 07:52:16.86 -32:23:16.5
248.26916 -2.69760 galactic Pup Second-epoch detections are separated by 1.0" and 5.5 pix
The object was found in VSX 4" GDS_J0752166-322318
Type: VAR
# Max. Min./Amp. JD0 Period
14.450 r Y 1.160 r M8
The object was not found in astcheck.
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 07:52:16.86 -32:23:16.5: 13.87 +/- 0.16 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 07:52:16.86 -32:23:16.5: 14.00 +/- 0.18 detection
Forced photometry reference-image weighted average: 13.93 +/- 0.12
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 Lite
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
GDS_J0752166-322318,2461347.9061,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J0752166-322318 20261103.4061 13.01CV 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 11 03.4061 2461347.9061 12.60 08:29:24.56 -35:29:56.3
255.08664 2.04041 galactic Pyx Second-epoch detections are separated by 1.4" and 4.9 pix
The object was found in VSX 2" GDS_J0829244-352956
Type: M
# Max. Min./Amp. JD0 Period
14.850 r Y 3.290 r 383.500000000000 S
The object was not found in astcheck.
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:29:24.56 -35:29:56.3: 14.78 +/- 99.00 upperlimit
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:29:24.56 -35:29:56.3: 14.74 +/- 99.00 upperlimit
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 Lite
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
GDS_J0829244-352956,2461347.9061,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J0829244-352956 20261103.4061 12.60CV 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 11 03.4061 2461347.9061 13.10 07:57:56.45 -30:22:00.0
247.16195 -0.61921 galactic Pup Second-epoch detections are separated by 4.2" and 5.2 pix
The object was found in VSX 1" GDS_J0757564-302159
Type: VAR
# Max. Min./Amp. JD0 Period
14.240 r Y 0.450 r M8
The object was not found in astcheck.
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 07:57:56.45 -30:22:00.0: 13.93 +/- 0.17 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 07:57:56.45 -30:22:00.0: 14.57 +/- 0.29 detection
Forced photometry reference-image weighted average: 14.09 +/- 0.15
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 Lite
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
GDS_J0757564-302159,2461347.9061,13.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J0757564-302159 20261103.4061 13.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 03.4061 2461347.9061 13.16 08:12:41.18 -34:04:59.7
251.97053 0.01969 galactic Pup Second-epoch detections are separated by 0.1" and 5.4 pix
The object was found in VSX 1" GDS_J0812412-340459
Type: M
# Max. Min./Amp. JD0 Period
13.900 r Y 2.540 r 494.700000000000 C
The object was not found in astcheck.
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:12:41.18 -34:04:59.7: 14.86 +/- 99.00 upperlimit
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:12:41.18 -34:04:59.7: 14.84 +/- 99.00 upperlimit
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 Lite
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
GDS_J0812412-340459,2461347.9061,13.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J0812412-340459 20261103.4061 13.16CV 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 11 03.4061 2461347.9061 13.37 08:18:50.99 -35:13:48.8
253.62914 0.43317 galactic Pup Second-epoch detections are separated by 0.6" and 5.4 pix
The object was found in VSX 2" OGLE-GD-LPV-000379
Type: M
# Max. Min./Amp. JD0 Period
11.789 Ic Y 4.119 Ic 426.200000000000
The object was not found in astcheck.
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:18:50.99 -35:13:48.8: 14.83 +/- 99.00 upperlimit
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:18:50.99 -35:13:48.8: 14.79 +/- 99.00 upperlimit
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 Lite
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
OGLE-GD-LPV-000379,2461347.9061,13.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
OGLE-GD-LPV-000379 20261103.4061 13.37CV 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 11 03.4061 2461347.9061 13.46 08:20:10.46 -35:16:42.2
253.82166 0.62906 galactic Pup Second-epoch detections are separated by 1.1" and 5.2 pix
The object was found in VSX 1" GDS_J0820103-351643
Type: VAR
# Max. Min./Amp. JD0 Period
13.510 r Y 0.390 r
The object was not found in astcheck.
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:20:10.46 -35:16:42.2: 14.36 +/- 0.23 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:20:10.46 -35:16:42.2: 14.47 +/- 0.25 detection
Forced photometry reference-image weighted average: 14.41 +/- 0.17
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 Lite
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
GDS_J0820103-351643,2461347.9061,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J0820103-351643 20261103.4061 13.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 03.4061 2461347.9061 12.63 08:25:48.37 -36:57:08.8
255.84544 0.60337 galactic Pup Second-epoch detections are separated by 4.2" and 5.0 pix
The object was found in VSX 1" GDS_J0825482-365707
Type: VAR
# Max. Min./Amp. JD0 Period
13.800 r Y 0.570 r M8
The object was not found in astcheck.
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:25:48.37 -36:57:08.8: 13.67 +/- 0.13 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:25:48.37 -36:57:08.8: 13.84 +/- 0.15 detection
Forced photometry reference-image weighted average: 13.74 +/- 0.10
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 Lite
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
GDS_J0825482-365707,2461347.9061,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J0825482-365707 20261103.4061 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 03.4061 2461347.9061 12.45 08:04:18.60 -36:22:27.1
252.96922 -2.65924 galactic Pup Second-epoch detections are separated by 1.8" and 5.6 pix
The object was found in VSX 2" GDS_J0804184-362227
Type: VAR
# Max. Min./Amp. JD0 Period
13.150 r Y 0.510 r
The object was not found in astcheck.
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:04:18.60 -36:22:27.1: 13.32 +/- 0.10 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:04:18.60 -36:22:27.1: 13.44 +/- 0.12 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.08
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 Lite
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
GDS_J0804184-362227,2461347.9061,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J0804184-362227 20261103.4061 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 03.4061 2461347.9061 11.70 08:11:13.06 -33:45:06.2
251.52614 -0.05281 galactic Pup Second-epoch detections are separated by 0.1" and 5.5 pix
The object was found in VSX 2" ASAS J081113-3345.1
Type: MISC
# Max. Min./Amp. JD0 Period
12.410 V Y 0.560 V 2452006.50000 51.770000000000
The object was not found in astcheck.
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:11:13.06 -33:45:06.2: 12.69 +/- 0.05 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:11:13.06 -33:45:06.2: 12.60 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.64 +/- 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 Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J081113-3345.1,2461347.9061,11.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J081113-3345.1 20261103.4061 11.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 03.4061 2461347.9061 12.36 08:42:35.92 -35:31:42.5
256.72268 4.17004 galactic Pyx Second-epoch detections are separated by 1.9" and 5.3 pix
The object was found in VSX 1" ASAS J084236-3531.7
Type: MISC
# Max. Min./Amp. JD0 Period
13.380 V Y 1.650 V 2452143.80000 120.600000000000
The object was not found in astcheck.
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:42:35.92 -35:31:42.5: 13.58 +/- 0.12 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:42:35.92 -35:31:42.5: 13.59 +/- 0.13 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J084236-3531.7,2461347.9061,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J084236-3531.7 20261103.4061 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 03.4061 2461347.9061 12.21 08:03:52.56 -38:36:11.0
254.81450 -3.91683 galactic Pup Second-epoch detections are separated by 0.6" and 5.0 pix
The object was found in VSX 2" ASAS J080353-3836.2
Type: M
# Max. Min./Amp. JD0 Period
13.214 V Y 2.132 V 2450006.32000 445.800000000000 C
The object was not found in astcheck.
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:03:52.56 -38:36:11.0: 13.49 +/- 0.12 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:03:52.56 -38:36:11.0: 13.51 +/- 0.13 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J080353-3836.2,2461347.9061,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J080353-3836.2 20261103.4061 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 03.4061 2461347.9061 12.21 08:29:03.43 -35:04:07.1
254.69540 2.23406 galactic Pyx Second-epoch detections are separated by 0.4" and 5.3 pix
The object was found in VSX 2" GDS_J0829033-350405
Type: VAR
# Max. Min./Amp. JD0 Period
13.120 r Y 0.870 r M7
The object was not found in astcheck.
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:29:03.43 -35:04:07.1: 13.53 +/- 0.11 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:29:03.43 -35:04:07.1: 13.29 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.07
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 Lite
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
GDS_J0829033-350405,2461347.9061,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J0829033-350405 20261103.4061 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 03.4061 2461347.9061 11.30 08:19:39.08 -37:20:06.6
255.45790 -0.62164 galactic Pup Second-epoch detections are separated by 0.6" and 5.1 pix
The object was found in VSX 0" ASAS J081939-3720.1
Type: MISC
# Max. Min./Amp. JD0 Period
8.916 Ic Y 0.186 Ic 2452950.70000 119.380000000000 M8
The object was not found in astcheck.
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:19:39.08 -37:20:06.6: 12.49 +/- 0.05 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:19:39.08 -37:20:06.6: 12.50 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.49 +/- 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 Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J081939-3720.1,2461347.9061,11.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J081939-3720.1 20261103.4061 11.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 03.4061 2461347.9061 11.49 08:48:37.59 -29:33:44.5
252.78385 8.84966 galactic Pyx Second-epoch detections are separated by 0.6" and 5.7 pix
The object was found in VSX 1" ASAS J084838-2933.7
Type: MISC|EC|E
# Max. Min./Amp. JD0 Period
10.640 V Y 0.910 V 2452062.50000 60.900000000000
The object was not found in astcheck.
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:48:37.59 -29:33:44.5: 12.42 +/- 0.04 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:48:37.59 -29:33:44.5: 12.48 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.45 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J084838-2933.7,2461347.9061,11.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J084838-2933.7 20261103.4061 11.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 03.4061 2461347.9061 12.38 07:58:41.43 -33:26:43.2
249.87086 -2.09225 galactic Pup Second-epoch detections are separated by 0.7" and 5.6 pix
The object was found in VSX 1" GDS_J0758413-332643
Type: VAR
# Max. Min./Amp. JD0 Period
12.700 r Y 0.660 r
The object was not found in astcheck.
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 07:58:41.43 -33:26:43.2: 13.37 +/- 0.10 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 07:58:41.43 -33:26:43.2: 13.26 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.07
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 Lite
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
GDS_J0758413-332643,2461347.9061,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J0758413-332643 20261103.4061 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 11 03.4061 2461347.9061 11.30 08:24:53.86 -32:10:06.0
251.82719 3.21047 galactic Pup Second-epoch detections are separated by 0.3" and 5.6 pix
The object was found in VSX 0" NSV 4064
Type: SR:
# Max. Min./Amp. JD0 Period
14.500 pg 15.900 pg 318.000000000000 Se
The object was not found in astcheck.
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:24:53.86 -32:10:06.0: 12.31 +/- 0.03 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:24:53.86 -32:10:06.0: 12.38 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.34 +/- 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 Lite
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
NSV 4064,2461347.9061,11.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSV 4064 20261103.4061 11.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 03.4061 2461347.9061 12.20 08:40:16.69 -36:02:10.9
256.83696 3.48709 galactic Pyx Second-epoch detections are separated by 3.5" and 4.5 pix
The object was found in VSX 1" GDS_J0840166-360211
Type: VAR
# Max. Min./Amp. JD0 Period
12.900 r Y 0.910 r
The object was not found in astcheck.
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:40:16.69 -36:02:10.9: 13.22 +/- 0.09 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:40:16.69 -36:02:10.9: 13.15 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.06
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 Lite
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
GDS_J0840166-360211,2461347.9061,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J0840166-360211 20261103.4061 12.20CV 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 11 03.4061 2461347.9061 11.12 08:19:08.23 -37:14:32.8
255.32362 -0.65368 galactic Pup Second-epoch detections are separated by 0.4" and 5.1 pix
The object was found in VSX 1" V0700 Pup
Type: M:
# Max. Min./Amp. JD0 Period
13.200 V < 14.500 V 2452810.00000 399.000000000000 : M9
The object was not found in astcheck.
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:19:08.23 -37:14:32.8: 12.08 +/- 0.03 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:19:08.23 -37:14:32.8: 12.13 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.11 +/- 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 Lite
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
V0700 Pup,2461347.9061,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0700 Pup 20261103.4061 11.12CV 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 11 03.4061 2461347.9061 10.80 07:58:56.11 -32:51:56.9
249.40346 -1.74547 galactic Pup Second-epoch detections are separated by 0.3" and 5.5 pix
The object was found in VSX 1" ASAS J075856-3252.0
Type: SR
# Max. Min./Amp. JD0 Period
8.473 Ic Y 0.270 Ic 2453097.30000 226.100000000000 M6
The object was not found in astcheck.
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 07:58:56.11 -32:51:56.9: 11.80 +/- 0.02 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 07:58:56.11 -32:51:56.9: 11.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.80 +/- 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 Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J075856-3252.0,2461347.9061,10.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J075856-3252.0 20261103.4061 10.80CV 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 11 03.4061 2461347.9061 11.90 08:13:51.85 -38:54:58.3
256.13347 -2.44885 galactic Pup Second-epoch detections are separated by 1.1" and 4.7 pix
The object was found in VSX 2" ASASSN-V J081351.81-385459.9
Type: L:
# Max. Min./Amp. JD0 Period
14.510 V 14.970 V
The object was not found in astcheck.
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:13:51.85 -38:54:58.3: 12.98 +/- 0.08 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:13:51.85 -38:54:58.3: 13.06 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
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 J081351.81-385459.9,2461347.9061,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J081351.81-385459.9 20261103.4061 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 11 03.4061 2461347.9061 11.91 08:26:59.23 -37:39:52.0
256.56171 0.38182 galactic Vel Second-epoch detections are separated by 1.4" and 5.0 pix
The object was found in VSX 4" ASAS J082659-3739.9
Type: SR
# Max. Min./Amp. JD0 Period
9.629 Ic Y 0.454 Ic 2454177.30000 484.000000000000 M9
The object was not found in astcheck.
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:26:59.23 -37:39:52.0: 13.01 +/- 0.07 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:26:59.23 -37:39:52.0: 13.10 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
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 11 03.4061* 08 26 59.23 -37 39 52.0 11.9 U Vel 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 J082659-3739.9,2461347.9061,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J082659-3739.9 20261103.4061 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 03.4061 2461347.9061 12.04 08:19:40.15 -36:15:03.6
254.56560 -0.00580 galactic Pup Second-epoch detections are separated by 1.8" and 5.4 pix
The object was found in VSX 0" GDS_J0819401-361503
Type: VAR
# Max. Min./Amp. JD0 Period
12.960 r Y 0.540 r M8
The object was not found in astcheck.
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:19:40.15 -36:15:03.6: 12.93 +/- 0.07 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:19:40.15 -36:15:03.6: 12.94 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
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
GDS_J0819401-361503,2461347.9061,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J0819401-361503 20261103.4061 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 11 03.4061 2461347.9061 12.00 08:38:22.51 -37:45:13.3
257.97096 2.14129 galactic Vel Second-epoch detections are separated by 1.2" and 4.8 pix
The object was found in VSX 1" GDS_J0838226-374513
Type: VAR
# Max. Min./Amp. JD0 Period
13.400 r Y 0.410 r M8
The object was not found in astcheck.
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:38:22.51 -37:45:13.3: 12.96 +/- 0.07 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:38:22.51 -37:45:13.3: 13.02 +/- 0.08 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
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 11 03.4061* 08 38 22.51 -37 45 13.3 12.0 U Vel 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
GDS_J0838226-374513,2461347.9061,12.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J0838226-374513 20261103.4061 12.00CV 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 11 03.4061 2461347.9061 11.97 08:50:35.40 -36:27:09.6
258.45780 4.85919 galactic Pyx Second-epoch detections are separated by 1.2" and 4.8 pix
The object was found in VSX 3" ASASSN-V J085035.64-362708.9
Type: SR
# Max. Min./Amp. JD0 Period
13.370 V 13.750 V 2457725.78200 62.170000000000
The object was not found in astcheck.
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:50:35.40 -36:27:09.6: 12.87 +/- 0.07 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:50:35.40 -36:27:09.6: 12.93 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
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 J085035.64-362708.9,2461347.9061,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J085035.64-362708.9 20261103.4061 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461136.59122270 06.04.2026 02:11:11.641 /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits
First image: 2461136.59122270 06.04.2026 02:11:11.641 /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits
Last image: 2461347.90639720 03.11.2026 09:45:02.718 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q1b1x1_034543_TTUQ1b1x1_1395907_ABJhZHwf/fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 44
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.29
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: 5 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 15173
Objects passed selection criteria: 15149
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 13578.5
Average stars matched: 13106.8 (96.5258 %)
Memory usage VmPeak: 239748 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Oct 15 15:05:03 CDT 2026
VaST build number 1.0rc89-241-g3eca6a38
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-15)
GNU bash, version 5.3.20(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Nov 3 03:52:57 CST 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: 2461136.59122270 06.04.2026 02:11:11.641 /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits
First image: 2461136.59122270 06.04.2026 02:11:11.641 /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits
Last image: 2461347.90639720 03.11.2026 09:45:02.718 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q1b1x1_034543_TTUQ1b1x1_1395907_ABJhZHwf/fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 159
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.94
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: 47 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 123273
Objects passed selection criteria: 123032
Measurements per detected object (mean, median, min, max): 3.2 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.2 4.0 2 4
Average stars detected per image: 105098
Average stars matched: 100817 (95.9274 %)
Memory usage VmPeak: 581804 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Oct 15 15:05:03 CDT 2026
VaST build number 1.0rc89-241-g3eca6a38
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-15)
GNU bash, version 5.3.20(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Nov 3 03:54:32 CST 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q1b1x1_034543_TTUQ1b1x1_1395907_ABJhZHwf/fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q1b1x1_034543_TTUQ1b1x1_1395907_ABJhZHwf/fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits
SExtractor catalog cache: saved Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits.cat to cache
SExtractor catalog cache: saved Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.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/Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q1b1x1_034543_TTUQ1b1x1_1395907_ABJhZHwf/fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q1b1x1_034543_TTUQ1b1x1_1395907_ABJhZHwf/fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits
Checking WCS cache directory local_wcs_cache
Checking 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: 2461347.90581687
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_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits exists and is non-empty
wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits exists and is non-empty
wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits exists and is non-empty
wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits (1st reference image)
verification OK: wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits
Image size: 937.3'x625.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 08:20:52.446 -34:00:38.17 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_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits (1st new image)
verification OK: wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits
Image size: 943.8'x627.9' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.90"/pix along the Y axis
Image center: 08:20:52.458 -34:00:31.96 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 08:20:52.446 -34:00:38.17
Second-epoch image center 08:20:52.458 -34:00:31.96
Angular distance between the image centers 0.0017 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits (2nd new image)
verification OK: wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits
Image size: 943.7'x627.9' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.90"/pix along the Y axis
Image center: 08:20:55.065 -34:00:33.36 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 08:20:52.446 -34:00:38.17
Second-epoch image center 08:20:55.065 -34:00:33.36
Angular distance between the image centers 0.0091 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 08:20:52.458 -34:00:31.96
Second-epoch second image center 08:20:55.065 -34:00:33.36
Angular distance between the image centers 0.00901 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/Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits &> /tmp/tmp.WdH4hA4iYV
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits &> /tmp/tmp.oYpiX2XeKj
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q1b1x1_034543_TTUQ1b1x1_1395907_ABJhZHwf/fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits &> /tmp/tmp.wrDCMNtdOj
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q1b1x1_034543_TTUQ1b1x1_1395907_ABJhZHwf/fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q1b1x1_034543_TTUQ1b1x1_1395907_ABJhZHwf/fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits &> /tmp/tmp.Kdr4BGdTI2
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q1b1x1_034543_TTUQ1b1x1_1395907_ABJhZHwf/fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits
Calibrating the magnitude scale
Found non-empty wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.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_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits and wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.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_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits and wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits.wcscat
Found non-empty wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits and wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits.wcscat
The reference image (wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits) and catalog (wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits.wcscat) found
'wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits.wcscat' -> 'wcsmag.cat'
Read 14942 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 115.3301 to 135.2911 deg, Dec -39.2872 to -28.4077 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 115.3301 to 135.2911 deg, Dec -39.2872 to -28.4077 deg
Loaded 26003 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): 11585 out of 12071 total matches.
Matched with Tycho-2 12071 out of 14942 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.597900
a=0.000000 b=1.000000 c=22.597900
From vast_summary.log: estimated ref. image limiting mag.: -8.29
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.31
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.31
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 14942 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 115.3301 to 135.2911 deg, Dec -39.2872 to -28.4077 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 115.3301 to 135.2911 deg, Dec -39.2872 to -28.4077 deg
Loaded 26003 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): 11585 out of 12071 total matches.
Matched with Tycho-2 12071 out of 14942 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits
Forced-photometry filter: calibrated wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits -> calib.txt_param_ref_wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits (aperture=6.3)
Read 15218 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 115.3104 to 135.2890 deg, Dec -39.2869 to -28.3706 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 115.3104 to 135.2890 deg, Dec -39.2869 to -28.3706 deg
Loaded 26108 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): 11747 out of 12249 total matches.
Matched with Tycho-2 12249 out of 15218 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits
Forced-photometry filter: calibrated wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits -> calib.txt_param_ref_wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits (aperture=6.3)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 42 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.4 pix Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits
2.4 pix Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits
3.5 pix fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits
3.5 pix fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits
Limiting magnitude estimates:
14.3 mag. Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits
14.3 mag. Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits
13.9 mag. fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits
13.9 mag. fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits
All-image limiting magnitude estimate: 13.9 (SNR ) 11.0 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.WdH4hA4iYV (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-11-03_CI_Pup-04-Q1b1x1_034543_TTUQ1b1x1_1395907_ABJhZHwf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits' -> 'wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits
WCS_IMAGE_NAME=wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits
WCS-calibrated image found: wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits
Checking if the catalog wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits.wcscat corresponding to the image wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits alredy exist and is non-empty...
Catalog wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits.wcscat corresponding to the image wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits
WCS catalog name: wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1211, bad_region=0, passed=14942
Got 14942 stars (including 13718 good ones) from the SExtractor catalog wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits.wcscat
util/solve_plate_with_UCAC5 got 14942 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 309 (Dec -39.3 to -28.4)
Done reading UCAC5 zone files...
Matched 4938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4862 matched stars entering correct_measured_positions(), 4862 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4862 matched stars entering correct_measured_positions(), 14942 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 309 (Dec -39.3 to -28.4)
Done reading UCAC5 zone files...
Matched 4938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4860 matched stars entering correct_measured_positions(), 14942 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Accuracy estimation diagnostic: 4860 matched stars entering correct_measured_positions(), 14942 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.74"
Excluding outliers - 4860 stars left (next iteration limit 5348)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits N_match=4860 sigma_overall_arcsec=0.698 sigma_q1_arcsec=0.485 sigma_q2_arcsec=1.009 sigma_q3_arcsec=0.682 sigma_q4_arcsec=0.879 n_q1=1198 n_q2=1136 n_q3=1349 n_q4=1177 worst_quadrant_to_overall_ratio=1.446
WCS_HEADER_DIAG: file=Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits selection=current_pairs N_selected=4860 N_valid=4860 bias_ra_arcsec=0.025 bias_dec_arcsec=0.007 median_sep_arcsec=0.489 p95_sep_arcsec=3.982 n_q1=1198 n_q2=1136 n_q3=1349 n_q4=1177 occupied_cells_4x4=16/16
The image catalog is written to wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits -region wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.oYpiX2XeKj (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-11-03_CI_Pup-04-Q1b1x1_034543_TTUQ1b1x1_1395907_ABJhZHwf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits' -> 'wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits
WCS_IMAGE_NAME=wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits
WCS-calibrated image found: wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits
Checking if the catalog wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits.wcscat corresponding to the image wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits alredy exist and is non-empty...
Catalog wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits.wcscat corresponding to the image wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits
WCS catalog name: wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1268, bad_region=0, passed=15218
Got 15218 stars (including 13937 good ones) from the SExtractor catalog wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits.wcscat
util/solve_plate_with_UCAC5 got 15218 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 310 (Dec -39.3 to -28.4)
Done reading UCAC5 zone files...
Matched 4938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4861 matched stars entering correct_measured_positions(), 4862 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4861 matched stars entering correct_measured_positions(), 15218 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 310 (Dec -39.3 to -28.4)
Done reading UCAC5 zone files...
Matched 4940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4860 matched stars entering correct_measured_positions(), 15218 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Accuracy estimation diagnostic: 4860 matched stars entering correct_measured_positions(), 15218 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
Excluding outliers - 4860 stars left (next iteration limit 5347)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits N_match=4860 sigma_overall_arcsec=0.689 sigma_q1_arcsec=0.520 sigma_q2_arcsec=0.938 sigma_q3_arcsec=0.639 sigma_q4_arcsec=0.888 n_q1=1199 n_q2=1131 n_q3=1347 n_q4=1183 worst_quadrant_to_overall_ratio=1.362
WCS_HEADER_DIAG: file=Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits selection=current_pairs N_selected=4860 N_valid=4860 bias_ra_arcsec=0.003 bias_dec_arcsec=0.012 median_sep_arcsec=0.497 p95_sep_arcsec=3.993 n_q1=1199 n_q2=1131 n_q3=1347 n_q4=1183 occupied_cells_4x4=16/16
The image catalog is written to wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits -region wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.wrDCMNtdOj (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_2026-11-03_CI_Pup-04-Q1b1x1_034543_TTUQ1b1x1_1395907_ABJhZHwf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q1b1x1_034543_TTUQ1b1x1_1395907_ABJhZHwf/fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q1b1x1_034543_TTUQ1b1x1_1395907_ABJhZHwf/fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q1b1x1_034543_TTUQ1b1x1_1395907_ABJhZHwf/fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q1b1x1_034543_TTUQ1b1x1_1395907_ABJhZHwf/fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q1b1x1_034543_TTUQ1b1x1_1395907_ABJhZHwf/fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.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_2026-11-03_CI_Pup-04-Q1b1x1_034543_TTUQ1b1x1_1395907_ABJhZHwf/fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits
WCS_IMAGE_NAME=wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits
WCS-calibrated image found: wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits
Checking if the catalog wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits.wcscat corresponding to the image wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits alredy exist and is non-empty...
Catalog wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits.wcscat corresponding to the image wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q1b1x1_034543_TTUQ1b1x1_1395907_ABJhZHwf/fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits
WCS catalog name: wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=660, bad_region=0, passed=12204
Got 12204 stars (including 11537 good ones) from the SExtractor catalog wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits.wcscat
util/solve_plate_with_UCAC5 got 12204 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 943.8'
Seting catalog search parameters based on the expected field of view 943.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013108 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010487 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 310 (Dec -39.3 to -28.2)
Done reading UCAC5 zone files...
Matched 4920 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4828 matched stars entering correct_measured_positions(), 4833 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4828 matched stars entering correct_measured_positions(), 12204 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 310 (Dec -39.3 to -28.2)
Done reading UCAC5 zone files...
Matched 4918 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4834 matched stars entering correct_measured_positions(), 12204 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Accuracy estimation diagnostic: 4834 matched stars entering correct_measured_positions(), 12204 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Excluding outliers - 4834 stars left (next iteration limit 5310)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4834 robust_rms=9.258 arcsec worst_region_rms=25.127 arcsec outer_annulus_rms=25.127 arcsec
SIP_REFIT: SIP order 3 trial: matched=4834 robust_rms=0.745 arcsec worst_region_rms=1.590 arcsec outer_annulus_rms=0.939 arcsec
SIP_REFIT: SIP order 5 trial: matched=4834 robust_rms=0.638 arcsec worst_region_rms=0.852 arcsec outer_annulus_rms=0.822 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4834 robust_rms_before=2.293 arcsec robust_rms_before_corrected=0.673 arcsec robust_rms_after=0.638 arcsec worst_region_rms_before=0.944 worst_region_rms_after=0.852 outer_annulus_rms_before=3.278 outer_annulus_rms_after=0.822
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.944 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits worst_region_rms_kept=0.944 arcsec robust_rms_kept=0.673 arcsec matched=4834
WCS_QUALITY_DIAG: file=fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits N_match=4834 sigma_overall_arcsec=0.640 sigma_q1_arcsec=0.681 sigma_q2_arcsec=0.853 sigma_q3_arcsec=0.523 sigma_q4_arcsec=0.603 n_q1=1201 n_q2=807 n_q3=1717 n_q4=1109 worst_quadrant_to_overall_ratio=1.332
WCS_HEADER_DIAG: file=fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits selection=current_pairs N_selected=4834 N_valid=4834 bias_ra_arcsec=0.853 bias_dec_arcsec=-0.441 median_sep_arcsec=1.909 p95_sep_arcsec=6.604 n_q1=1201 n_q2=807 n_q3=1717 n_q4=1109 occupied_cells_4x4=16/16
The image catalog is written to wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q1b1x1_034543_TTUQ1b1x1_1395907_ABJhZHwf/fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits -region wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.Kdr4BGdTI2 (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_2026-11-03_CI_Pup-04-Q1b1x1_034543_TTUQ1b1x1_1395907_ABJhZHwf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q1b1x1_034543_TTUQ1b1x1_1395907_ABJhZHwf/fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q1b1x1_034543_TTUQ1b1x1_1395907_ABJhZHwf/fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q1b1x1_034543_TTUQ1b1x1_1395907_ABJhZHwf/fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q1b1x1_034543_TTUQ1b1x1_1395907_ABJhZHwf/fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q1b1x1_034543_TTUQ1b1x1_1395907_ABJhZHwf/fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.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_2026-11-03_CI_Pup-04-Q1b1x1_034543_TTUQ1b1x1_1395907_ABJhZHwf/fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits
WCS_IMAGE_NAME=wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits
WCS-calibrated image found: wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits
Checking if the catalog wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits.wcscat corresponding to the image wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits alredy exist and is non-empty...
Catalog wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits.wcscat corresponding to the image wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q1b1x1_034543_TTUQ1b1x1_1395907_ABJhZHwf/fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits
WCS catalog name: wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=667, bad_region=0, passed=12289
Got 12289 stars (including 11615 good ones) from the SExtractor catalog wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits.wcscat
util/solve_plate_with_UCAC5 got 12289 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 943.7'
Seting catalog search parameters based on the expected field of view 943.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013107 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010486 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 310 (Dec -39.3 to -28.2)
Done reading UCAC5 zone files...
Matched 4922 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4830 matched stars entering correct_measured_positions(), 4836 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4830 matched stars entering correct_measured_positions(), 12289 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 310 (Dec -39.3 to -28.2)
Done reading UCAC5 zone files...
Matched 4920 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4834 matched stars entering correct_measured_positions(), 12289 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Accuracy estimation diagnostic: 4834 matched stars entering correct_measured_positions(), 12289 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Excluding outliers - 4834 stars left (next iteration limit 5313)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4834 robust_rms=9.429 arcsec worst_region_rms=24.866 arcsec outer_annulus_rms=24.866 arcsec
SIP_REFIT: SIP order 3 trial: matched=4834 robust_rms=0.753 arcsec worst_region_rms=2.110 arcsec outer_annulus_rms=0.949 arcsec
SIP_REFIT: SIP order 5 trial: matched=4834 robust_rms=0.652 arcsec worst_region_rms=0.998 arcsec outer_annulus_rms=0.838 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4834 robust_rms_before=2.495 arcsec robust_rms_before_corrected=0.670 arcsec robust_rms_after=0.652 arcsec worst_region_rms_before=0.938 worst_region_rms_after=0.998 outer_annulus_rms_before=4.068 outer_annulus_rms_after=0.838
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.938 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits worst_region_rms_kept=0.938 arcsec robust_rms_kept=0.670 arcsec matched=4834
WCS_QUALITY_DIAG: file=fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits N_match=4834 sigma_overall_arcsec=0.631 sigma_q1_arcsec=0.671 sigma_q2_arcsec=0.923 sigma_q3_arcsec=0.538 sigma_q4_arcsec=0.584 n_q1=1206 n_q2=820 n_q3=1702 n_q4=1106 worst_quadrant_to_overall_ratio=1.461
WCS_HEADER_DIAG: file=fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits selection=current_pairs N_selected=4834 N_valid=4834 bias_ra_arcsec=0.862 bias_dec_arcsec=-0.440 median_sep_arcsec=2.086 p95_sep_arcsec=7.237 n_q1=1206 n_q2=820 n_q3=1702 n_q4=1106 occupied_cells_4x4=16/16
The image catalog is written to wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q1b1x1_034543_TTUQ1b1x1_1395907_ABJhZHwf/fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits -region wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Saving the final (post-refit) wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits to local_wcs_cache/
'wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits' -> 'local_wcs_cache/wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits'
Saving the final (post-refit) wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits to local_wcs_cache/
'wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits' -> 'local_wcs_cache/wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits'
Saving the final (post-refit) wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits to local_wcs_cache/
'wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits' -> 'local_wcs_cache/wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits'
Saving the final (post-refit) wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits to local_wcs_cache/
'wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits' -> 'local_wcs_cache/wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits sigma_overall=0.698 worst_q_ratio=1.446
ref2=Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits sigma_overall=0.689 worst_q_ratio=1.362
new1=fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits sigma_overall=0.640 worst_q_ratio=1.332
new2=fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits sigma_overall=0.631 worst_q_ratio=1.461
reference average sigma_overall=0.6935 worst_q_ratio=1.404
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010_astrometric_residuals.png (4860 matched stars from wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.66 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011_astrometric_residuals.png (4860 matched stars from wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.66 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455_astrometric_residuals.png (4834 matched stars from wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.60 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456_astrometric_residuals.png (4834 matched stars from wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.61 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q1b1x1_034543_TTUQ1b1x1_1395907_ABJhZHwf/wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits'
Saving fully-calibrated image wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q1b1x1_034543_TTUQ1b1x1_1395907_ABJhZHwf/wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits'
Preparing the HTML report for the field Pup-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 07:58:56.09 -32:51:57.0: 11.69 +/- 0.03 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:41:00.81 -39:04:56.4: 99.00 +/- 99.00 edge
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:52:07.17 -38:52:43.9: 99.00 +/- 99.00 edge
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:20:50.41 -28:58:38.7: 10.97 +/- 0.01 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 07:50:25.90 -29:14:25.5: 11.44 +/- 0.03 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:02:28.91 -32:19:05.0: 11.21 +/- 0.02 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:03:19.29 -31:38:01.5: 11.68 +/- 0.02 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:21:10.03 -32:33:09.2: 11.52 +/- 0.02 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 07:52:38.72 -30:07:05.1: 11.73 +/- 0.03 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:20:50.41 -28:58:38.7: 10.93 +/- 0.01 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:41:00.81 -39:04:56.4: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 08:41:00.81 -39:04:56.4: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry reference-image weighted average: 10.95 +/- 0.01
Forced photometry filter REJECTED candidate at 08:20:50.41 -28:58:38.7: ref_mag=10.95 +/- 0.01 new_mean_mag=10.9759 delta=-0.02 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 07:58:56.09 -32:51:57.0: 11.66 +/- 0.02 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:52:07.17 -38:52:43.9: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 08:52:07.17 -38:52:43.9: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry reference-image weighted average: 11.68 +/- 0.02
Forced photometry filter REJECTED candidate at 07:58:56.09 -32:51:57.0: ref_mag=11.68 +/- 0.02 new_mean_mag=10.8007 delta=0.88 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:03:19.29 -31:38:01.5: 11.68 +/- 0.02 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:02:28.91 -32:19:05.0: 11.23 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.22 +/- 0.01
Forced photometry reference-image weighted average: 11.68 +/- 0.02
Forced photometry filter REJECTED candidate at 08:02:28.91 -32:19:05.0: ref_mag=11.22 +/- 0.01 new_mean_mag=11.1644 delta=0.06 (need > 0.90)
Forced photometry filter REJECTED candidate at 08:03:19.29 -31:38:01.5: ref_mag=11.68 +/- 0.02 new_mean_mag=11.0730 delta=0.60 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 07:52:38.72 -30:07:05.1: 11.73 +/- 0.03 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:21:10.03 -32:33:09.2: 11.53 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.53 +/- 0.01
Forced photometry reference-image weighted average: 11.73 +/- 0.02
Forced photometry filter REJECTED candidate at 07:52:38.72 -30:07:05.1: ref_mag=11.73 +/- 0.02 new_mean_mag=11.2254 delta=0.50 (need > 0.90)
Forced photometry filter REJECTED candidate at 08:21:10.03 -32:33:09.2: ref_mag=11.53 +/- 0.01 new_mean_mag=10.9765 delta=0.55 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 07:50:25.90 -29:14:25.5: 11.42 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.43 +/- 0.02
Forced photometry filter REJECTED candidate at 07:50:25.90 -29:14:25.5: ref_mag=11.43 +/- 0.02 new_mean_mag=11.2251 delta=0.20 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:21:50.38 -36:07:31.2: 11.74 +/- 0.02 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:24:48.57 -33:07:31.7: 11.69 +/- 0.02 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 07:45:23.95 -31:54:46.4: 11.33 +/- 0.02 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:31:32.09 -30:37:47.8: 11.53 +/- 0.02 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:11:26.83 -34:42:46.4: 11.57 +/- 0.02 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:13:11.52 -31:53:54.6: 11.20 +/- 0.01 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:21:50.38 -36:07:31.2: 11.70 +/- 0.02 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 07:59:34.29 -30:10:34.2: 11.33 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.72 +/- 0.02
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:04:46.23 -32:30:11.6: 11.20 +/- 0.02 detection
Forced photometry filter REJECTED candidate at 08:21:50.38 -36:07:31.2: ref_mag=11.72 +/- 0.02 new_mean_mag=10.9014 delta=0.82 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:33:29.20 -32:38:24.9: 11.55 +/- 0.02 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:24:48.57 -33:07:31.7: 11.71 +/- 0.02 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:31:32.09 -30:37:47.8: 11.56 +/- 0.02 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 07:45:23.95 -31:54:46.4: 11.30 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.70 +/- 0.02
Forced photometry reference-image weighted average: 11.54 +/- 0.01
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:11:26.83 -34:42:46.4: 11.57 +/- 0.02 detection
Forced photometry filter REJECTED candidate at 08:24:48.57 -33:07:31.7: ref_mag=11.70 +/- 0.02 new_mean_mag=10.9921 delta=0.71 (need > 0.90)
Forced photometry filter REJECTED candidate at 08:31:32.09 -30:37:47.8: ref_mag=11.54 +/- 0.01 new_mean_mag=11.0779 delta=0.46 (need > 0.90)
Forced photometry reference-image weighted average: 11.31 +/- 0.01
Forced photometry filter REJECTED candidate at 07:45:23.95 -31:54:46.4: ref_mag=11.31 +/- 0.01 new_mean_mag=11.2890 delta=0.03 (need > 0.90)
Forced photometry reference-image weighted average: 11.57 +/- 0.01
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:13:11.52 -31:53:54.6: 11.24 +/- 0.02 detection
Forced photometry filter REJECTED candidate at 08:11:26.83 -34:42:46.4: ref_mag=11.57 +/- 0.01 new_mean_mag=11.0729 delta=0.49 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 07:59:34.29 -30:10:34.2: 11.32 +/- 0.02 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:04:46.23 -32:30:11.6: 11.16 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.22 +/- 0.01
Forced photometry reference-image weighted average: 11.33 +/- 0.01
Forced photometry filter REJECTED candidate at 08:13:11.52 -31:53:54.6: ref_mag=11.22 +/- 0.01 new_mean_mag=11.1627 delta=0.06 (need > 0.90)
Forced photometry filter REJECTED candidate at 07:59:34.29 -30:10:34.2: ref_mag=11.33 +/- 0.01 new_mean_mag=11.3045 delta=0.02 (need > 0.90)
Forced photometry reference-image weighted average: 11.18 +/- 0.01
Forced photometry filter REJECTED candidate at 08:04:46.23 -32:30:11.6: ref_mag=11.18 +/- 0.01 new_mean_mag=11.2213 delta=-0.04 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:22:30.26 -31:18:40.8: 11.39 +/- 0.02 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:33:29.20 -32:38:24.9: 11.51 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.53 +/- 0.01
Forced photometry filter REJECTED candidate at 08:33:29.20 -32:38:24.9: ref_mag=11.53 +/- 0.01 new_mean_mag=11.0640 delta=0.46 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:15:53.74 -29:29:16.3: 11.45 +/- 0.02 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:22:30.26 -31:18:40.8: 11.40 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.39 +/- 0.01
Forced photometry filter REJECTED candidate at 08:22:30.26 -31:18:40.8: ref_mag=11.39 +/- 0.01 new_mean_mag=11.1901 delta=0.20 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:13:01.72 -31:18:00.5: 11.30 +/- 0.02 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 07:59:12.21 -34:33:25.0: 11.55 +/- 0.02 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:17:44.31 -30:03:59.8: 11.50 +/- 0.02 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:28:23.48 -30:33:48.5: 11.36 +/- 0.02 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:39:19.74 -30:05:26.4: 11.34 +/- 0.02 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:20:09.43 -29:54:52.1: 11.33 +/- 0.02 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:26:50.89 -30:39:36.0: 11.34 +/- 0.02 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:15:53.74 -29:29:16.3: 11.42 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.43 +/- 0.01
Forced photometry filter REJECTED candidate at 08:15:53.74 -29:29:16.3: ref_mag=11.43 +/- 0.01 new_mean_mag=11.2942 delta=0.14 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:13:01.72 -31:18:00.5: 11.28 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.29 +/- 0.01
Forced photometry filter REJECTED candidate at 08:13:01.72 -31:18:00.5: ref_mag=11.29 +/- 0.01 new_mean_mag=11.3036 delta=-0.01 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 07:59:12.21 -34:33:25.0: 11.52 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.54 +/- 0.01
Forced photometry filter REJECTED candidate at 07:59:12.21 -34:33:25.0: ref_mag=11.54 +/- 0.01 new_mean_mag=11.3478 delta=0.19 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:17:44.31 -30:03:59.8: 11.47 +/- 0.02 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:39:19.74 -30:05:26.4: 11.32 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.48 +/- 0.01
Forced photometry filter REJECTED candidate at 08:17:44.31 -30:03:59.8: ref_mag=11.48 +/- 0.01 new_mean_mag=11.2758 delta=0.21 (need > 0.90)
Forced photometry reference-image weighted average: 11.33 +/- 0.01
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:26:50.89 -30:39:36.0: 11.34 +/- 0.02 detection
Forced photometry filter REJECTED candidate at 08:39:19.74 -30:05:26.4: ref_mag=11.33 +/- 0.01 new_mean_mag=11.2842 delta=0.05 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:20:09.43 -29:54:52.1: 11.32 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.34 +/- 0.01
Forced photometry filter REJECTED candidate at 08:26:50.89 -30:39:36.0: ref_mag=11.34 +/- 0.01 new_mean_mag=11.3061 delta=0.03 (need > 0.90)
Forced photometry reference-image weighted average: 11.32 +/- 0.01
Forced photometry filter REJECTED candidate at 08:20:09.43 -29:54:52.1: ref_mag=11.32 +/- 0.01 new_mean_mag=11.2732 delta=0.05 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:28:23.48 -30:33:48.5: 11.34 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.35 +/- 0.01
Forced photometry filter REJECTED candidate at 08:28:23.48 -30:33:48.5: ref_mag=11.35 +/- 0.01 new_mean_mag=11.3442 delta=0.01 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:35:04.68 -35:29:50.9: 11.16 +/- 0.02 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:18:45.59 -31:51:11.9: 11.35 +/- 0.02 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:23:04.30 -38:48:29.5: 8.79 +/- 0.00 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:35:04.68 -35:29:50.9: 11.15 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.15 +/- 0.01
Forced photometry filter REJECTED candidate at 08:35:04.68 -35:29:50.9: ref_mag=11.15 +/- 0.01 new_mean_mag=10.5182 delta=0.63 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 07:52:07.16 -38:34:56.1: 10.77 +/- 0.02 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:18:45.59 -31:51:11.9: 11.31 +/- 0.02 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:23:04.30 -38:48:29.5: 8.79 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.33 +/- 0.01
Forced photometry reference-image weighted average: 8.79 +/- 0.00
Forced photometry filter KEPT candidate at 08:18:45.59 -31:51:11.9: ref_mag=11.33 +/- 0.01 new_mean_mag=10.2613 delta=1.07 (need > 0.90)
Forced photometry filter KEPT candidate at 08:23:04.30 -38:48:29.5: ref_mag=8.79 +/- 0.00 new_mean_mag=7.8627 delta=0.93 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 07:52:07.16 -38:34:56.1: 10.76 +/- 0.02 detection
Forced photometry reference-image weighted average: 10.76 +/- 0.02
Forced photometry filter REJECTED candidate at 07:52:07.16 -38:34:56.1: ref_mag=10.76 +/- 0.02 new_mean_mag=10.4097 delta=0.35 (need > 0.90)
Adding exclusion_list_local.txt__out00540.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09994.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 21035_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 21035_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
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Considering the candidate 21062_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 21062_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
**** FOUND 08:08:56.52 -37:28:15.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21108_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 21108_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
**** FOUND 08:43:12.01 -33:05:45.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21175_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 21175_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
**** FOUND 08:04:27.15 -35:15:12.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21219_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 21219_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
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Considering the candidate 21250_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 21250_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
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Considering the candidate 21252_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 21252_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
**** FOUND 08:23:19.28 -35:24:57.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21263_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 21263_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21266_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 21266_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
**** FOUND 08:52:54.20 -29:33:58.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21297_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 21297_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
**** FOUND 07:51:20.78 -29:07:26.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21323_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 21323_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21339_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 21339_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21342_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 21342_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21349_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 21349_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21357_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 21357_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
**** FOUND 08:43:19.33 -29:56:56.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21362_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 21362_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21363_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 21363_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
**** FOUND 08:07:49.88 -35:54:00.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21365_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 21365_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21367_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 21367_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21369_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 21369_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21370_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 21370_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21371_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 21371_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21375_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 21375_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21378_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 21378_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21389_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 21389_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21390_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 21390_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
**** FOUND 08:12:30.54 -30:09:04.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21399_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 21399_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21400_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 21400_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21401_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 21401_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21404_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 21404_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21420_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 21420_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21433_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 21433_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21461_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 21461_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21480_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 21480_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21485_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 21485_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21492_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 21492_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08857_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 08857_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
**** FOUND 08:07:03.56 -32:38:45.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08675_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 08675_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
**** FOUND 08:43:41.02 -32:31:40.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 04811_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 04811_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09994_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
Preparing report for the candidate 09994_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 00540_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
Preparing report for the candidate 00540_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 00754_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 00754_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 7s
Prepared the HTML report for the field Pup-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
08:23:04.30 -38:48:29.5
08:18:45.59 -31:51:11.9
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/Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q1b1x1_034543_TTUQ1b1x1_1395907_ABJhZHwf/fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q1b1x1_034543_TTUQ1b1x1_1395907_ABJhZHwf/fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits
SExtractor catalog cache: saved Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits.cat to cache
SExtractor catalog cache: saved Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q1b1x1_034543_TTUQ1b1x1_1395907_ABJhZHwf/fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q1b1x1_034543_TTUQ1b1x1_1395907_ABJhZHwf/fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits
Creating symlink local_wcs_cache/wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits
Creating symlink local_wcs_cache/wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits
Creating symlink local_wcs_cache/wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits
Checking 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_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits exists and is non-empty
wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits exists and is non-empty
wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits exists and is non-empty
wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits (1st reference image)
verification OK: wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits
Image size: 937.3'x625.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 08:20:52.446 -34:00:38.17 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_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits (1st new image)
verification OK: wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits
Image size: 943.8'x627.9' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.90"/pix along the Y axis
Image center: 08:20:52.458 -34:00:31.96 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 08:20:52.446 -34:00:38.17
Second-epoch image center 08:20:52.458 -34:00:31.96
Angular distance between the image centers 0.0017 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits (2nd new image)
verification OK: wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits
Image size: 943.7'x627.9' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.90"/pix along the Y axis
Image center: 08:20:55.065 -34:00:33.36 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 08:20:52.446 -34:00:38.17
Second-epoch image center 08:20:55.065 -34:00:33.36
Angular distance between the image centers 0.0091 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 08:20:52.458 -34:00:31.96
Second-epoch second image center 08:20:55.065 -34:00:33.36
Angular distance between the image centers 0.00901 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/Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits &> /tmp/tmp.ZLWkfTk9I2
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits &> /tmp/tmp.c6jbsLEcp7
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q1b1x1_034543_TTUQ1b1x1_1395907_ABJhZHwf/fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits &> /tmp/tmp.ZCb1YUfYTC
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q1b1x1_034543_TTUQ1b1x1_1395907_ABJhZHwf/fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q1b1x1_034543_TTUQ1b1x1_1395907_ABJhZHwf/fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits &> /tmp/tmp.atqF6HKF2f
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q1b1x1_034543_TTUQ1b1x1_1395907_ABJhZHwf/fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits
Calibrating the magnitude scale
Found non-empty wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.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_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits and wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.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_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits and wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits.wcscat
Found non-empty wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits and wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits.wcscat
The reference image (wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits) and catalog (wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits.wcscat) found
'wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits.wcscat' -> 'wcsmag.cat'
Read 132037 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 115.3025 to 135.3575 deg, Dec -39.2952 to -28.3517 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 115.3025 to 135.3575 deg, Dec -39.2952 to -28.3517 deg
Loaded 26236 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): 17756 out of 21157 total matches.
Matched with Tycho-2 21157 out of 132037 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.410050
a=0.000000 b=1.000000 c=22.410050
From vast_summary.log: estimated ref. image limiting mag.: -7.94
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.47
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.47
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 132037 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 115.3025 to 135.3575 deg, Dec -39.2952 to -28.3517 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 115.3025 to 135.3575 deg, Dec -39.2952 to -28.3517 deg
Loaded 26236 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): 17756 out of 21157 total matches.
Matched with Tycho-2 21157 out of 132037 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits
Forced-photometry filter: calibrated wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits -> calib.txt_param_ref_wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits (aperture=4.7)
Read 134376 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 115.3028 to 135.3209 deg, Dec -39.2901 to -28.3510 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 115.3028 to 135.3209 deg, Dec -39.2901 to -28.3510 deg
Loaded 26201 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): 17706 out of 21125 total matches.
Matched with Tycho-2 21125 out of 134376 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits
Forced-photometry filter: calibrated wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits -> calib.txt_param_ref_wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits (aperture=4.7)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 140 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits
2.1 pix Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits
3.4 pix fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits
3.4 pix fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits
Limiting magnitude estimates:
14.5 mag. Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits
14.5 mag. Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits
13.9 mag. fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits
13.9 mag. fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits
All-image limiting magnitude estimate: 13.9 (SNR ) 13.0 (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.ZLWkfTk9I2 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-11-03_CI_Pup-04-Q1b1x1_034543_TTUQ1b1x1_1395907_ABJhZHwf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits' -> 'wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits
WCS_IMAGE_NAME=wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits
WCS-calibrated image found: wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits
Checking if the catalog wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits.wcscat corresponding to the image wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits alredy exist and is non-empty...
Catalog wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits.wcscat corresponding to the image wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits
WCS catalog name: wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=22, blended=12979, bad_region=0, passed=132015
Got 132015 stars (including 118905 good ones) from the SExtractor catalog wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits.wcscat
util/solve_plate_with_UCAC5 got 132015 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 310 (Dec -39.3 to -28.4)
Done reading UCAC5 zone files...
Matched 4932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4875 matched stars entering correct_measured_positions(), 4875 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4875 matched stars entering correct_measured_positions(), 132015 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 310 (Dec -39.3 to -28.4)
Done reading UCAC5 zone files...
Matched 4931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4876 matched stars entering correct_measured_positions(), 132015 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Accuracy estimation diagnostic: 4876 matched stars entering correct_measured_positions(), 132015 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Excluding outliers - 4876 stars left (next iteration limit 5362)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits N_match=4876 sigma_overall_arcsec=0.684 sigma_q1_arcsec=0.490 sigma_q2_arcsec=0.931 sigma_q3_arcsec=0.668 sigma_q4_arcsec=0.939 n_q1=1276 n_q2=1110 n_q3=1290 n_q4=1200 worst_quadrant_to_overall_ratio=1.372
WCS_HEADER_DIAG: file=Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits selection=current_pairs N_selected=4876 N_valid=4876 bias_ra_arcsec=0.035 bias_dec_arcsec=0.016 median_sep_arcsec=0.485 p95_sep_arcsec=3.490 n_q1=1276 n_q2=1110 n_q3=1290 n_q4=1200 occupied_cells_4x4=16/16
The image catalog is written to wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits -region wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.c6jbsLEcp7 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-11-03_CI_Pup-04-Q1b1x1_034543_TTUQ1b1x1_1395907_ABJhZHwf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits' -> 'wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits
WCS_IMAGE_NAME=wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits
WCS-calibrated image found: wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits
Checking if the catalog wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits.wcscat corresponding to the image wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits alredy exist and is non-empty...
Catalog wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits.wcscat corresponding to the image wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits
WCS catalog name: wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=32, blended=13323, bad_region=0, passed=134344
Got 134344 stars (including 120867 good ones) from the SExtractor catalog wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits.wcscat
util/solve_plate_with_UCAC5 got 134344 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 310 (Dec -39.3 to -28.4)
Done reading UCAC5 zone files...
Matched 4932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4873 matched stars entering correct_measured_positions(), 4873 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4873 matched stars entering correct_measured_positions(), 134344 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 310 (Dec -39.3 to -28.4)
Done reading UCAC5 zone files...
Matched 4934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4871 matched stars entering correct_measured_positions(), 134344 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Accuracy estimation diagnostic: 4871 matched stars entering correct_measured_positions(), 134344 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Excluding outliers - 4871 stars left (next iteration limit 5360)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits N_match=4871 sigma_overall_arcsec=0.669 sigma_q1_arcsec=0.486 sigma_q2_arcsec=0.898 sigma_q3_arcsec=0.643 sigma_q4_arcsec=0.916 n_q1=1277 n_q2=1112 n_q3=1287 n_q4=1195 worst_quadrant_to_overall_ratio=1.369
WCS_HEADER_DIAG: file=Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits selection=current_pairs N_selected=4871 N_valid=4871 bias_ra_arcsec=0.021 bias_dec_arcsec=0.014 median_sep_arcsec=0.492 p95_sep_arcsec=3.466 n_q1=1277 n_q2=1112 n_q3=1287 n_q4=1195 occupied_cells_4x4=16/16
The image catalog is written to wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits -region wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.ZCb1YUfYTC (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_2026-11-03_CI_Pup-04-Q1b1x1_034543_TTUQ1b1x1_1395907_ABJhZHwf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q1b1x1_034543_TTUQ1b1x1_1395907_ABJhZHwf/fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q1b1x1_034543_TTUQ1b1x1_1395907_ABJhZHwf/fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q1b1x1_034543_TTUQ1b1x1_1395907_ABJhZHwf/fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q1b1x1_034543_TTUQ1b1x1_1395907_ABJhZHwf/fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q1b1x1_034543_TTUQ1b1x1_1395907_ABJhZHwf/fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.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_2026-11-03_CI_Pup-04-Q1b1x1_034543_TTUQ1b1x1_1395907_ABJhZHwf/fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits
WCS_IMAGE_NAME=wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits
WCS-calibrated image found: wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits
Checking if the catalog wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits.wcscat corresponding to the image wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits alredy exist and is non-empty...
Catalog wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits.wcscat corresponding to the image wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q1b1x1_034543_TTUQ1b1x1_1395907_ABJhZHwf/fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits
WCS catalog name: wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=6525, bad_region=19, passed=78496
Got 78496 stars (including 71865 good ones) from the SExtractor catalog wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits.wcscat
util/solve_plate_with_UCAC5 got 78496 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 943.8'
Seting catalog search parameters based on the expected field of view 943.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013108 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010487 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 311 (Dec -39.4 to -28.2)
Done reading UCAC5 zone files...
Matched 4916 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4840 matched stars entering correct_measured_positions(), 4842 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4840 matched stars entering correct_measured_positions(), 78496 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 311 (Dec -39.4 to -28.2)
Done reading UCAC5 zone files...
Matched 4918 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4848 matched stars entering correct_measured_positions(), 78496 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Accuracy estimation diagnostic: 4848 matched stars entering correct_measured_positions(), 78496 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Excluding outliers - 4848 stars left (next iteration limit 5324)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4848 robust_rms=9.672 arcsec worst_region_rms=25.065 arcsec outer_annulus_rms=25.065 arcsec
SIP_REFIT: SIP order 3 trial: matched=4848 robust_rms=0.746 arcsec worst_region_rms=1.590 arcsec outer_annulus_rms=0.936 arcsec
SIP_REFIT: SIP order 5 trial: matched=4848 robust_rms=0.639 arcsec worst_region_rms=0.856 arcsec outer_annulus_rms=0.825 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4848 robust_rms_before=2.291 arcsec robust_rms_before_corrected=0.657 arcsec robust_rms_after=0.639 arcsec worst_region_rms_before=0.939 worst_region_rms_after=0.856 outer_annulus_rms_before=3.245 outer_annulus_rms_after=0.825
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.939 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits worst_region_rms_kept=0.939 arcsec robust_rms_kept=0.657 arcsec matched=4848
WCS_QUALITY_DIAG: file=fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits N_match=4848 sigma_overall_arcsec=0.624 sigma_q1_arcsec=0.684 sigma_q2_arcsec=0.839 sigma_q3_arcsec=0.509 sigma_q4_arcsec=0.590 n_q1=1201 n_q2=798 n_q3=1711 n_q4=1138 worst_quadrant_to_overall_ratio=1.346
WCS_HEADER_DIAG: file=fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits selection=current_pairs N_selected=4848 N_valid=4848 bias_ra_arcsec=0.874 bias_dec_arcsec=-0.488 median_sep_arcsec=1.903 p95_sep_arcsec=6.199 n_q1=1201 n_q2=798 n_q3=1711 n_q4=1138 occupied_cells_4x4=16/16
The image catalog is written to wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q1b1x1_034543_TTUQ1b1x1_1395907_ABJhZHwf/fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits -region wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.atqF6HKF2f (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_2026-11-03_CI_Pup-04-Q1b1x1_034543_TTUQ1b1x1_1395907_ABJhZHwf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q1b1x1_034543_TTUQ1b1x1_1395907_ABJhZHwf/fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q1b1x1_034543_TTUQ1b1x1_1395907_ABJhZHwf/fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q1b1x1_034543_TTUQ1b1x1_1395907_ABJhZHwf/fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q1b1x1_034543_TTUQ1b1x1_1395907_ABJhZHwf/fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q1b1x1_034543_TTUQ1b1x1_1395907_ABJhZHwf/fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.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_2026-11-03_CI_Pup-04-Q1b1x1_034543_TTUQ1b1x1_1395907_ABJhZHwf/fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits
WCS_IMAGE_NAME=wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits
WCS-calibrated image found: wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits
Checking if the catalog wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits.wcscat corresponding to the image wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits alredy exist and is non-empty...
Catalog wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits.wcscat corresponding to the image wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q1b1x1_034543_TTUQ1b1x1_1395907_ABJhZHwf/fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits
WCS catalog name: wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=1, no_mag_err=0, low_SNR=5, blended=6596, bad_region=22, passed=78672
Got 78672 stars (including 71963 good ones) from the SExtractor catalog wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits.wcscat
util/solve_plate_with_UCAC5 got 78672 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 943.7'
Seting catalog search parameters based on the expected field of view 943.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013107 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010486 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 311 (Dec -39.4 to -28.2)
Done reading UCAC5 zone files...
Matched 4921 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4845 matched stars entering correct_measured_positions(), 4846 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4845 matched stars entering correct_measured_positions(), 78672 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 311 (Dec -39.4 to -28.2)
Done reading UCAC5 zone files...
Matched 4920 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4855 matched stars entering correct_measured_positions(), 78672 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Accuracy estimation diagnostic: 4855 matched stars entering correct_measured_positions(), 78671 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Excluding outliers - 4855 stars left (next iteration limit 5329)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4855 robust_rms=9.679 arcsec worst_region_rms=24.580 arcsec outer_annulus_rms=24.580 arcsec
SIP_REFIT: SIP order 3 trial: matched=4855 robust_rms=0.758 arcsec worst_region_rms=2.098 arcsec outer_annulus_rms=0.924 arcsec
SIP_REFIT: SIP order 5 trial: matched=4855 robust_rms=0.651 arcsec worst_region_rms=0.999 arcsec outer_annulus_rms=0.822 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4855 robust_rms_before=2.508 arcsec robust_rms_before_corrected=0.660 arcsec robust_rms_after=0.651 arcsec worst_region_rms_before=0.917 worst_region_rms_after=0.999 outer_annulus_rms_before=3.949 outer_annulus_rms_after=0.822
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.917 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits worst_region_rms_kept=0.917 arcsec robust_rms_kept=0.660 arcsec matched=4855
WCS_QUALITY_DIAG: file=fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits N_match=4855 sigma_overall_arcsec=0.621 sigma_q1_arcsec=0.676 sigma_q2_arcsec=0.901 sigma_q3_arcsec=0.513 sigma_q4_arcsec=0.596 n_q1=1201 n_q2=806 n_q3=1723 n_q4=1125 worst_quadrant_to_overall_ratio=1.452
WCS_HEADER_DIAG: file=fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits selection=current_pairs N_selected=4855 N_valid=4855 bias_ra_arcsec=0.872 bias_dec_arcsec=-0.473 median_sep_arcsec=2.102 p95_sep_arcsec=7.031 n_q1=1201 n_q2=806 n_q3=1723 n_q4=1125 occupied_cells_4x4=16/16
The image catalog is written to wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q1b1x1_034543_TTUQ1b1x1_1395907_ABJhZHwf/fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits -region wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
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_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.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_2026-11-03_CI_Pup-04-Q1b1x1_034543_TTUQ1b1x1_1395907_ABJhZHwf/wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-44-12_20.00sec_-0.00C_LIGHTs_0455.fits
Saving fully-calibrated image wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.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_2026-11-03_CI_Pup-04-Q1b1x1_034543_TTUQ1b1x1_1395907_ABJhZHwf/wcs_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456.fits
Preparing the HTML report for the field Pup-04-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:39:15.84 -32:15:27.5: 12.55 +/- 0.04 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:35:26.35 -33:50:28.4: 13.26 +/- 0.09 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:06:32.13 -29:52:04.1: 12.82 +/- 0.06 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:10:49.95 -31:07:17.1: 12.95 +/- 0.07 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 07:59:53.30 -31:42:47.9: 12.85 +/- 0.06 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:26:16.38 -32:53:30.8: 12.88 +/- 0.06 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:18:37.68 -33:38:10.7: 14.26 +/- 0.21 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:24:27.14 -35:37:53.0: 12.44 +/- 0.04 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 07:58:23.81 -31:34:10.7: 13.12 +/- 0.07 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:35:00.98 -37:01:35.7: 12.96 +/- 0.07 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:39:15.84 -32:15:27.5: 12.50 +/- 0.04 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:35:26.35 -33:50:28.4: 13.44 +/- 0.10 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:18:37.68 -33:38:10.7: 14.44 +/- 0.25 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:06:32.13 -29:52:04.1: 12.78 +/- 0.06 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:10:49.95 -31:07:17.1: 12.92 +/- 0.06 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 07:59:53.30 -31:42:47.9: 12.88 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.07
Forced photometry reference-image weighted average: 12.52 +/- 0.03
Forced photometry reference-image weighted average: 14.34 +/- 0.16
Forced photometry reference-image weighted average: 12.80 +/- 0.05
Forced photometry filter REJECTED candidate at 08:35:26.35 -33:50:28.4: ref_mag=13.33 +/- 0.07 new_mean_mag=13.0273 delta=0.31 (need > 0.90)
Forced photometry filter KEPT candidate at 08:18:37.68 -33:38:10.7: ref_mag=14.34 +/- 0.16 new_mean_mag=12.9700 delta=1.37 (need > 0.90)
Forced photometry filter REJECTED candidate at 08:39:15.84 -32:15:27.5: ref_mag=12.52 +/- 0.03 new_mean_mag=12.7096 delta=-0.18 (need > 0.90)
Forced photometry filter REJECTED candidate at 08:06:32.13 -29:52:04.1: ref_mag=12.80 +/- 0.05 new_mean_mag=13.0026 delta=-0.20 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:26:16.38 -32:53:30.8: 12.77 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.04
Forced photometry reference-image weighted average: 12.86 +/- 0.04
Forced photometry filter REJECTED candidate at 08:10:49.95 -31:07:17.1: ref_mag=12.93 +/- 0.04 new_mean_mag=13.1963 delta=-0.26 (need > 0.90)
Forced photometry filter REJECTED candidate at 07:59:53.30 -31:42:47.9: ref_mag=12.86 +/- 0.04 new_mean_mag=12.6673 delta=0.20 (need > 0.90)
Forced photometry reference-image weighted average: 12.82 +/- 0.04
Forced photometry filter REJECTED candidate at 08:26:16.38 -32:53:30.8: ref_mag=12.82 +/- 0.04 new_mean_mag=12.7800 delta=0.04 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:24:27.14 -35:37:53.0: 12.41 +/- 0.04 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:35:00.98 -37:01:35.7: 13.07 +/- 0.08 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 07:58:23.81 -31:34:10.7: 13.05 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.43 +/- 0.03
Forced photometry reference-image weighted average: 13.01 +/- 0.05
Forced photometry filter REJECTED candidate at 08:24:27.14 -35:37:53.0: ref_mag=12.43 +/- 0.03 new_mean_mag=12.5693 delta=-0.14 (need > 0.90)
Forced photometry filter REJECTED candidate at 08:35:00.98 -37:01:35.7: ref_mag=13.01 +/- 0.05 new_mean_mag=12.4341 delta=0.57 (need > 0.90)
Forced photometry reference-image weighted average: 13.09 +/- 0.05
Forced photometry filter REJECTED candidate at 07:58:23.81 -31:34:10.7: ref_mag=13.09 +/- 0.05 new_mean_mag=12.9096 delta=0.18 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:09:38.45 -30:25:59.3: 12.95 +/- 0.07 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:10:57.25 -36:35:18.7: 12.86 +/- 0.08 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:54:25.14 -29:49:24.0: 12.20 +/- 0.04 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 07:46:24.11 -30:51:03.8: 12.75 +/- 0.07 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:22:28.36 -37:28:47.4: 11.75 +/- 0.02 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:26:13.03 -32:57:46.3: 12.07 +/- 0.03 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:52:07.14 -38:52:43.8: 99.00 +/- 99.00 edge
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:09:38.45 -30:25:59.3: 12.86 +/- 0.06 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:10:57.25 -36:35:18.7: 12.91 +/- 0.08 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.05
Forced photometry reference-image weighted average: 12.88 +/- 0.05
Forced photometry filter REJECTED candidate at 08:09:38.45 -30:25:59.3: ref_mag=12.90 +/- 0.05 new_mean_mag=12.9415 delta=-0.04 (need > 0.90)
Forced photometry filter REJECTED candidate at 08:10:57.25 -36:35:18.7: ref_mag=12.88 +/- 0.05 new_mean_mag=12.4820 delta=0.40 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:54:25.14 -29:49:24.0: 12.18 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.19 +/- 0.03
Forced photometry filter REJECTED candidate at 08:54:25.14 -29:49:24.0: ref_mag=12.19 +/- 0.03 new_mean_mag=12.2496 delta=-0.06 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:22:28.36 -37:28:47.4: 11.79 +/- 0.02 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 07:46:24.11 -30:51:03.8: 12.67 +/- 0.06 detection
Forced photometry reference-image weighted average: 11.77 +/- 0.02
Forced photometry filter REJECTED candidate at 08:22:28.36 -37:28:47.4: ref_mag=11.77 +/- 0.02 new_mean_mag=11.9030 delta=-0.13 (need > 0.90)
Forced photometry reference-image weighted average: 12.71 +/- 0.05
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:26:13.03 -32:57:46.3: 12.12 +/- 0.03 detection
Forced photometry filter REJECTED candidate at 07:46:24.11 -30:51:03.8: ref_mag=12.71 +/- 0.05 new_mean_mag=12.6488 delta=0.06 (need > 0.90)
Forced photometry reference-image weighted average: 12.10 +/- 0.02
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:41:00.86 -39:04:55.5: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 08:26:13.03 -32:57:46.3: ref_mag=12.10 +/- 0.02 new_mean_mag=12.0527 delta=0.04 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:52:07.14 -38:52:43.8: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 08:52:07.14 -38:52:43.8: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:41:00.86 -39:04:55.5: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 08:41:00.86 -39:04:55.5: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:46:45.31 -38:59:23.5: 99.00 +/- 99.00 edge
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:57:35.00 -38:35:59.0: 11.60 +/- 0.03 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:55:02.68 -38:49:19.3: 99.00 +/- 99.00 edge
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:58:47.81 -38:35:08.5: 12.06 +/- 0.04 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:17:07.59 -31:26:38.4: 10.96 +/- 0.01 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:46:45.31 -38:59:23.5: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 08:46:45.31 -38:59:23.5: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:57:35.00 -38:35:59.0: 11.61 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.60 +/- 0.02
Forced photometry filter REJECTED candidate at 08:57:35.00 -38:35:59.0: ref_mag=11.60 +/- 0.02 new_mean_mag=11.4128 delta=0.19 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:55:02.68 -38:49:19.3: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 08:55:02.68 -38:49:19.3: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:58:47.81 -38:35:08.5: 12.10 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.08 +/- 0.03
Forced photometry filter REJECTED candidate at 08:58:47.81 -38:35:08.5: ref_mag=12.08 +/- 0.03 new_mean_mag=11.7077 delta=0.37 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:17:07.59 -31:26:38.4: 11.00 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.98 +/- 0.01
Forced photometry filter REJECTED candidate at 08:17:07.59 -31:26:38.4: ref_mag=10.98 +/- 0.01 new_mean_mag=12.4008 delta=-1.42 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:38:56.82 -29:19:55.4: 12.68 +/- 0.05 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:24:42.77 -32:26:53.0: 14.85 +/- 0.34 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:01:58.37 -35:08:27.9: 12.60 +/- 0.06 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:53:16.46 -38:51:37.2: 99.00 +/- 99.00 edge
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:38:56.82 -29:19:55.4: 12.74 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.04
Forced photometry filter REJECTED candidate at 08:38:56.82 -29:19:55.4: ref_mag=12.71 +/- 0.04 new_mean_mag=12.5776 delta=0.13 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 07:46:19.65 -29:36:04.4: 13.58 +/- 0.18 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:24:42.77 -32:26:53.0: 14.88 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.85 +/- 0.34
Forced photometry filter KEPT candidate at 08:24:42.77 -32:26:53.0: ref_mag=14.85 +/- 0.34 new_mean_mag=12.6934 delta=2.15 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:01:58.37 -35:08:27.9: 12.71 +/- 0.06 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:29:24.56 -35:29:56.3: 14.78 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.66 +/- 0.04
Forced photometry filter REJECTED candidate at 08:01:58.37 -35:08:27.9: ref_mag=12.66 +/- 0.04 new_mean_mag=12.6365 delta=0.02 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:53:16.46 -38:51:37.2: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 08:53:16.46 -38:51:37.2: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 07:52:16.86 -32:23:16.5: 13.87 +/- 0.16 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:17:05.17 -31:25:20.9: 12.59 +/- 0.06 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 07:46:19.65 -29:36:04.4: 13.86 +/- 0.22 detection
Forced photometry reference-image weighted average: 13.69 +/- 0.14
Forced photometry filter REJECTED candidate at 07:46:19.65 -29:36:04.4: ref_mag=13.69 +/- 0.14 new_mean_mag=13.1990 delta=0.49 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:29:24.56 -35:29:56.3: 14.74 +/- 99.00 upperlimit
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 07:52:16.86 -32:23:16.5: 14.00 +/- 0.18 detection
Forced photometry reference-image weighted average: 13.93 +/- 0.12
Forced photometry filter KEPT candidate at 07:52:16.86 -32:23:16.5: ref_mag=13.93 +/- 0.12 new_mean_mag=13.0102 delta=0.92 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 07:57:56.45 -30:22:00.0: 13.93 +/- 0.17 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:17:05.17 -31:25:20.9: 12.53 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.56 +/- 0.04
Forced photometry filter REJECTED candidate at 08:17:05.17 -31:25:20.9: ref_mag=12.56 +/- 0.04 new_mean_mag=12.9515 delta=-0.39 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 07:57:56.45 -30:22:00.0: 14.57 +/- 0.29 detection
Forced photometry reference-image weighted average: 14.09 +/- 0.15
Forced photometry filter KEPT candidate at 07:57:56.45 -30:22:00.0: ref_mag=14.09 +/- 0.15 new_mean_mag=13.0907 delta=1.00 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 07:57:21.36 -32:29:45.1: 13.75 +/- 0.17 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 07:47:39.45 -35:32:23.2: 13.65 +/- 0.14 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:16:59.60 -32:59:53.8: 12.81 +/- 0.06 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 07:54:30.60 -32:28:34.3: 13.09 +/- 0.08 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 07:57:21.36 -32:29:45.1: 13.62 +/- 0.15 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.11
Forced photometry filter REJECTED candidate at 07:57:21.36 -32:29:45.1: ref_mag=13.68 +/- 0.11 new_mean_mag=13.2410 delta=0.44 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:12:41.18 -34:04:59.7: 14.86 +/- 99.00 upperlimit
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 07:47:39.45 -35:32:23.2: 13.67 +/- 0.14 detection
Forced photometry reference-image weighted average: 13.66 +/- 0.10
Forced photometry filter REJECTED candidate at 07:47:39.45 -35:32:23.2: ref_mag=13.66 +/- 0.10 new_mean_mag=13.0826 delta=0.58 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:16:59.60 -32:59:53.8: 12.95 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.87 +/- 0.05
Forced photometry filter REJECTED candidate at 08:16:59.60 -32:59:53.8: ref_mag=12.87 +/- 0.05 new_mean_mag=12.9760 delta=-0.11 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 07:54:30.60 -32:28:34.3: 13.04 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.05
Forced photometry filter REJECTED candidate at 07:54:30.60 -32:28:34.3: ref_mag=13.07 +/- 0.05 new_mean_mag=13.0261 delta=0.04 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:12:41.18 -34:04:59.7: 14.84 +/- 99.00 upperlimit
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 07:52:13.05 -30:05:36.1: 13.88 +/- 0.22 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 07:51:20.38 -29:55:20.2: 13.73 +/- 0.15 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:10:36.92 -29:46:34.3: 13.67 +/- 0.12 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 07:52:13.05 -30:05:36.1: 13.65 +/- 0.17 detection
Forced photometry reference-image weighted average: 13.74 +/- 0.13
Forced photometry filter REJECTED candidate at 07:52:13.05 -30:05:36.1: ref_mag=13.74 +/- 0.13 new_mean_mag=13.4755 delta=0.26 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 07:51:20.38 -29:55:20.2: 13.83 +/- 0.16 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:10:36.92 -29:46:34.3: 13.68 +/- 0.12 detection
Forced photometry reference-image weighted average: 13.78 +/- 0.11
Forced photometry reference-image weighted average: 13.67 +/- 0.08
Forced photometry filter REJECTED candidate at 07:51:20.38 -29:55:20.2: ref_mag=13.78 +/- 0.11 new_mean_mag=13.3746 delta=0.41 (need > 0.90)
Forced photometry filter REJECTED candidate at 08:10:36.92 -29:46:34.3: ref_mag=13.67 +/- 0.08 new_mean_mag=13.4018 delta=0.27 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:26:46.37 -32:08:09.6: 13.88 +/- 0.15 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 07:49:15.62 -28:43:42.8: 13.60 +/- 0.17 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 07:46:51.89 -29:19:41.5: 13.94 +/- 0.20 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:33:46.37 -37:35:17.3: 13.70 +/- 0.14 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:26:46.37 -32:08:09.6: 13.79 +/- 0.14 detection
Forced photometry reference-image weighted average: 13.83 +/- 0.10
Forced photometry filter REJECTED candidate at 08:26:46.37 -32:08:09.6: ref_mag=13.83 +/- 0.10 new_mean_mag=13.0709 delta=0.76 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 07:49:15.62 -28:43:42.8: 13.85 +/- 0.21 detection
Forced photometry reference-image weighted average: 13.70 +/- 0.13
Forced photometry filter REJECTED candidate at 07:49:15.62 -28:43:42.8: ref_mag=13.70 +/- 0.13 new_mean_mag=13.6255 delta=0.07 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 07:46:51.89 -29:19:41.5: 13.79 +/- 0.17 detection
Forced photometry reference-image weighted average: 13.85 +/- 0.13
Forced photometry filter REJECTED candidate at 07:46:51.89 -29:19:41.5: ref_mag=13.85 +/- 0.13 new_mean_mag=13.4996 delta=0.35 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:33:46.37 -37:35:17.3: 13.93 +/- 0.17 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.11
Forced photometry filter REJECTED candidate at 08:33:46.37 -37:35:17.3: ref_mag=13.79 +/- 0.11 new_mean_mag=12.9079 delta=0.88 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 07:46:51.59 -28:57:49.1: 13.85 +/- 0.20 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:03:08.63 -32:46:24.5: 14.13 +/- 0.18 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:07:36.86 -28:49:37.3: 13.86 +/- 0.15 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 07:46:51.59 -28:57:49.1: 13.79 +/- 0.17 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.13
Forced photometry filter REJECTED candidate at 07:46:51.59 -28:57:49.1: ref_mag=13.81 +/- 0.13 new_mean_mag=13.5375 delta=0.28 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 07:55:35.27 -32:17:20.5: 14.32 +/- 0.25 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:03:08.63 -32:46:24.5: 14.34 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.22 +/- 0.14
Forced photometry filter REJECTED candidate at 08:03:08.63 -32:46:24.5: ref_mag=14.22 +/- 0.14 new_mean_mag=13.4026 delta=0.82 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:07:36.86 -28:49:37.3: 13.73 +/- 0.12 detection
Forced photometry reference-image weighted average: 13.78 +/- 0.09
Forced photometry filter REJECTED candidate at 08:07:36.86 -28:49:37.3: ref_mag=13.78 +/- 0.09 new_mean_mag=13.4597 delta=0.32 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 07:55:35.27 -32:17:20.5: 14.13 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.21 +/- 0.16
Forced photometry filter REJECTED candidate at 07:55:35.27 -32:17:20.5: ref_mag=14.21 +/- 0.16 new_mean_mag=13.3708 delta=0.84 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 07:56:36.60 -30:34:28.9: 13.81 +/- 0.16 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 07:52:07.88 -29:51:14.5: 13.85 +/- 0.17 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 07:56:36.60 -30:34:28.9: 13.87 +/- 0.17 detection
Forced photometry reference-image weighted average: 13.84 +/- 0.12
Forced photometry filter REJECTED candidate at 07:56:36.60 -30:34:28.9: ref_mag=13.84 +/- 0.12 new_mean_mag=13.5588 delta=0.28 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 07:59:46.29 -29:38:07.4: 14.12 +/- 0.22 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 07:48:29.40 -28:57:38.2: 14.48 +/- 0.33 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 07:52:07.88 -29:51:14.5: 13.90 +/- 0.18 detection
Forced photometry reference-image weighted average: 13.87 +/- 0.12
Forced photometry filter REJECTED candidate at 07:52:07.88 -29:51:14.5: ref_mag=13.87 +/- 0.12 new_mean_mag=13.6251 delta=0.25 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 07:59:46.29 -29:38:07.4: 14.19 +/- 0.23 detection
Forced photometry reference-image weighted average: 14.15 +/- 0.16
Forced photometry filter REJECTED candidate at 07:59:46.29 -29:38:07.4: ref_mag=14.15 +/- 0.16 new_mean_mag=13.6969 delta=0.45 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 07:48:29.40 -28:57:38.2: 13.71 +/- 0.16 detection
Forced photometry reference-image weighted average: 13.85 +/- 0.14
Forced photometry filter REJECTED candidate at 07:48:29.40 -28:57:38.2: ref_mag=13.85 +/- 0.14 new_mean_mag=13.7095 delta=0.14 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 07:48:26.38 -30:26:38.6: 13.83 +/- 0.20 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 07:47:51.70 -28:54:52.2: 14.06 +/- 0.23 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 07:48:26.38 -30:26:38.6: 13.70 +/- 0.17 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 07:47:51.70 -28:54:52.2: 13.81 +/- 0.18 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:02:41.24 -35:41:52.3: 14.19 +/- 0.21 detection
Forced photometry reference-image weighted average: 13.76 +/- 0.13
Forced photometry filter REJECTED candidate at 07:48:26.38 -30:26:38.6: ref_mag=13.76 +/- 0.13 new_mean_mag=13.5675 delta=0.19 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 07:47:38.12 -30:30:56.7: 13.60 +/- 0.15 detection
Forced photometry reference-image weighted average: 13.90 +/- 0.14
Forced photometry filter REJECTED candidate at 07:47:51.70 -28:54:52.2: ref_mag=13.90 +/- 0.14 new_mean_mag=13.6746 delta=0.23 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:02:41.24 -35:41:52.3: 14.06 +/- 0.18 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 07:47:38.12 -30:30:56.7: 13.64 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.11 +/- 0.14
Forced photometry filter REJECTED candidate at 08:02:41.24 -35:41:52.3: ref_mag=14.11 +/- 0.14 new_mean_mag=13.3698 delta=0.75 (need > 0.90)
Forced photometry reference-image weighted average: 13.62 +/- 0.11
Forced photometry filter REJECTED candidate at 07:47:38.12 -30:30:56.7: ref_mag=13.62 +/- 0.11 new_mean_mag=13.7411 delta=-0.12 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:26:04.17 -29:29:18.0: 13.78 +/- 0.13 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:26:04.17 -29:29:18.0: 13.86 +/- 0.14 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:18:50.99 -35:13:48.8: 14.83 +/- 99.00 upperlimit
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:20:10.46 -35:16:42.2: 14.36 +/- 0.23 detection
Forced photometry reference-image weighted average: 13.82 +/- 0.10
Forced photometry filter REJECTED candidate at 08:26:04.17 -29:29:18.0: ref_mag=13.82 +/- 0.10 new_mean_mag=13.5124 delta=0.30 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:20:10.46 -35:16:42.2: 14.47 +/- 0.25 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:18:50.99 -35:13:48.8: 14.79 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.41 +/- 0.17
Forced photometry filter KEPT candidate at 08:20:10.46 -35:16:42.2: ref_mag=14.41 +/- 0.17 new_mean_mag=13.4550 delta=0.95 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:25:48.37 -36:57:08.8: 13.67 +/- 0.13 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:25:48.37 -36:57:08.8: 13.84 +/- 0.15 detection
Forced photometry reference-image weighted average: 13.74 +/- 0.10
Forced photometry filter KEPT candidate at 08:25:48.37 -36:57:08.8: ref_mag=13.74 +/- 0.10 new_mean_mag=12.6090 delta=1.14 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:04:18.60 -36:22:27.1: 13.32 +/- 0.10 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:04:18.60 -36:22:27.1: 13.44 +/- 0.12 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.08
Forced photometry filter KEPT candidate at 08:04:18.60 -36:22:27.1: ref_mag=13.37 +/- 0.08 new_mean_mag=12.4443 delta=0.93 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:11:13.06 -33:45:06.2: 12.69 +/- 0.05 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:11:13.06 -33:45:06.2: 12.60 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.64 +/- 0.03
Forced photometry filter KEPT candidate at 08:11:13.06 -33:45:06.2: ref_mag=12.64 +/- 0.03 new_mean_mag=11.6961 delta=0.94 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:42:35.92 -35:31:42.5: 13.58 +/- 0.12 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:42:35.92 -35:31:42.5: 13.59 +/- 0.13 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:03:52.56 -38:36:11.0: 13.49 +/- 0.12 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.09
Forced photometry filter KEPT candidate at 08:42:35.92 -35:31:42.5: ref_mag=13.59 +/- 0.09 new_mean_mag=12.3436 delta=1.24 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:03:52.56 -38:36:11.0: 13.51 +/- 0.13 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.09
Forced photometry filter KEPT candidate at 08:03:52.56 -38:36:11.0: ref_mag=13.50 +/- 0.09 new_mean_mag=12.2054 delta=1.29 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:29:03.43 -35:04:07.1: 13.53 +/- 0.11 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:29:03.43 -35:04:07.1: 13.29 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.07
Forced photometry filter KEPT candidate at 08:29:03.43 -35:04:07.1: ref_mag=13.38 +/- 0.07 new_mean_mag=12.2002 delta=1.18 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:07:17.22 -31:54:23.7: 13.40 +/- 0.09 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:19:39.08 -37:20:06.6: 12.49 +/- 0.05 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:48:37.59 -29:33:44.5: 12.42 +/- 0.04 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:07:17.22 -31:54:23.7: 13.37 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.07
Forced photometry filter REJECTED candidate at 08:07:17.22 -31:54:23.7: ref_mag=13.38 +/- 0.07 new_mean_mag=12.4871 delta=0.90 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:19:39.08 -37:20:06.6: 12.50 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.49 +/- 0.03
Forced photometry filter KEPT candidate at 08:19:39.08 -37:20:06.6: ref_mag=12.49 +/- 0.03 new_mean_mag=11.3016 delta=1.19 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:48:37.59 -29:33:44.5: 12.48 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.45 +/- 0.03
Forced photometry filter KEPT candidate at 08:48:37.59 -29:33:44.5: ref_mag=12.45 +/- 0.03 new_mean_mag=11.4926 delta=0.95 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 07:58:41.43 -33:26:43.2: 13.37 +/- 0.10 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 07:58:41.43 -33:26:43.2: 13.26 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.07
Forced photometry filter KEPT candidate at 07:58:41.43 -33:26:43.2: ref_mag=13.30 +/- 0.07 new_mean_mag=12.3835 delta=0.92 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:24:53.86 -32:10:06.0: 12.31 +/- 0.03 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:24:53.86 -32:10:06.0: 12.38 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.34 +/- 0.02
Forced photometry filter KEPT candidate at 08:24:53.86 -32:10:06.0: ref_mag=12.34 +/- 0.02 new_mean_mag=11.2962 delta=1.04 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:40:16.69 -36:02:10.9: 13.22 +/- 0.09 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:40:16.69 -36:02:10.9: 13.15 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.06
Forced photometry filter KEPT candidate at 08:40:16.69 -36:02:10.9: ref_mag=13.18 +/- 0.06 new_mean_mag=12.1932 delta=0.99 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:19:08.23 -37:14:32.8: 12.08 +/- 0.03 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:19:08.23 -37:14:32.8: 12.13 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.11 +/- 0.02
Forced photometry filter KEPT candidate at 08:19:08.23 -37:14:32.8: ref_mag=12.11 +/- 0.02 new_mean_mag=11.1202 delta=0.99 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:18:14.26 -37:54:49.2: 12.37 +/- 0.05 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:18:14.26 -37:54:49.2: 12.33 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.35 +/- 0.03
Forced photometry filter REJECTED candidate at 08:18:14.26 -37:54:49.2: ref_mag=12.35 +/- 0.03 new_mean_mag=12.0366 delta=0.31 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 07:58:56.11 -32:51:56.9: 11.80 +/- 0.02 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 07:58:56.11 -32:51:56.9: 11.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.80 +/- 0.02
Forced photometry filter KEPT candidate at 07:58:56.11 -32:51:56.9: ref_mag=11.80 +/- 0.02 new_mean_mag=10.8088 delta=0.99 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:13:51.85 -38:54:58.3: 12.98 +/- 0.08 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:26:59.23 -37:39:52.0: 13.01 +/- 0.07 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:58:38.86 -36:32:13.6: 12.48 +/- 0.05 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:19:40.15 -36:15:03.6: 12.93 +/- 0.07 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:13:51.85 -38:54:58.3: 13.06 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.05
Forced photometry filter KEPT candidate at 08:13:51.85 -38:54:58.3: ref_mag=13.02 +/- 0.05 new_mean_mag=11.9055 delta=1.12 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:26:59.23 -37:39:52.0: 13.10 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.05
Forced photometry filter KEPT candidate at 08:26:59.23 -37:39:52.0: ref_mag=13.05 +/- 0.05 new_mean_mag=11.9017 delta=1.15 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:58:38.86 -36:32:13.6: 12.53 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.50 +/- 0.04
Forced photometry filter REJECTED candidate at 08:58:38.86 -36:32:13.6: ref_mag=12.50 +/- 0.04 new_mean_mag=12.0896 delta=0.41 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:19:40.15 -36:15:03.6: 12.94 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.05
Forced photometry filter KEPT candidate at 08:19:40.15 -36:15:03.6: ref_mag=12.93 +/- 0.05 new_mean_mag=12.0225 delta=0.91 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:58:06.76 -35:21:25.1: 12.26 +/- 0.04 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:38:22.51 -37:45:13.3: 12.96 +/- 0.07 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:58:06.76 -35:21:25.1: 12.30 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.28 +/- 0.03
Forced photometry filter REJECTED candidate at 08:58:06.76 -35:21:25.1: ref_mag=12.28 +/- 0.03 new_mean_mag=11.9246 delta=0.35 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:38:22.51 -37:45:13.3: 13.02 +/- 0.08 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.05
Forced photometry filter KEPT candidate at 08:38:22.51 -37:45:13.3: ref_mag=12.99 +/- 0.05 new_mean_mag=11.9939 delta=0.99 (need > 0.90)
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:50:35.40 -36:27:09.6: 12.87 +/- 0.07 detection
Forced photometry on wcs_Pup-04-Q1b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:50:35.40 -36:27:09.6: 12.93 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.05
Forced photometry filter KEPT candidate at 08:50:35.40 -36:27:09.6: ref_mag=12.90 +/- 0.05 new_mean_mag=11.9649 delta=0.93 (need > 0.90)
Adding exclusion_list_local.txt__out02313.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04288.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09320.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10979.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14083.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out142862.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out143439.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14890.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out155987.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out157555.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out157769.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out157849.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out157879.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out158143.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out158526.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out158557.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19210.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25062.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25519.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out30394.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37293.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55630.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out59166.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67959.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out78633.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out89944.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 63s
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: 15s
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Considering the candidate 155974_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 155974_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
**** FOUND 08:11:22.57 -29:23:41.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 155979_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 155979_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
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Considering the candidate 155980_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 155980_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
Rejecting candidate due to large distance (18.2") between the two second-epoch detections
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Considering the candidate 155982_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 155982_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
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Considering the candidate 155984_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 155984_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
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Considering the candidate 155987_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
Preparing report for the candidate 155987_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
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Considering the candidate 155988_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 155988_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
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Considering the candidate 155991_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 155991_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
**** FOUND 07:51:39.98 -31:10:42.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 156000_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 156000_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
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Considering the candidate 156010_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 156010_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
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Considering the candidate 156011_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 156011_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
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Considering the candidate 156012_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 156012_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
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Considering the candidate 156013_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 156013_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
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Considering the candidate 156014_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 156014_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
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Considering the candidate 156016_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 156016_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
**** FOUND 08:54:05.24 -33:13:07.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 156018_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 156018_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
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Considering the candidate 156019_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 156019_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
**** FOUND 08:47:08.14 -29:11:25.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 156020_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 156020_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
**** FOUND 07:57:00.19 -30:15:49.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 156025_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 156025_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
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Considering the candidate 156026_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 156026_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
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Considering the candidate 156028_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 156028_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
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Considering the candidate 156029_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 156029_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
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Considering the candidate 156052_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 156052_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
**** FOUND 08:57:44.14 -38:44:39.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 156233_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 156233_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
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Considering the candidate 156268_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 156268_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
**** FOUND 08:52:54.16 -29:33:59.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 156272_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 156272_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
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Considering the candidate 156294_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 156294_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
**** FOUND 07:51:20.79 -29:07:26.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 156359_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 156359_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
**** FOUND 08:07:49.90 -35:54:00.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 156394_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 156394_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
**** FOUND 08:06:08.31 -37:17:45.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 156649_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 156649_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
**** FOUND 07:45:27.28 -37:58:07.5 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 156697_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 156697_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
**** FOUND 08:30:39.11 -31:20:26.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 156708_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 156708_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
**** FOUND 08:10:48.91 -32:52:06.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 156729_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 156729_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
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Considering the candidate 156738_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 156738_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
Rejecting candidate due to large distance (27.9") between the two second-epoch detections
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Considering the candidate 156789_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 156789_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
**** FOUND 08:20:20.97 -32:13:57.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 156866_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 156866_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
**** FOUND 08:21:22.70 -33:05:08.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 156898_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 156898_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
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Considering the candidate 156915_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 156915_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
**** FOUND 08:47:31.02 -38:48:37.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 156942_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 156942_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
Rejecting candidate due to large distance (30.4") between the two second-epoch detections
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Considering the candidate 156952_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 156952_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
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Considering the candidate 157135_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 157135_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
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Considering the candidate 157204_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 157204_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
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Considering the candidate 157208_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 157208_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
**** FOUND 08:26:25.21 -33:12:37.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 157214_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 157214_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
**** FOUND 07:52:19.41 -31:47:57.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 157222_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 157222_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
**** FOUND 08:00:10.68 -29:31:37.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 157349_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 157349_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
**** FOUND 08:18:58.05 -29:43:55.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 157399_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 157399_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
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Considering the candidate 157466_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 157466_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
Rejecting candidate due to large distance (29.3") between the two second-epoch detections
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Considering the candidate 157495_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 157495_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
**** FOUND 08:02:32.66 -30:14:12.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 157550_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 157550_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
**** FOUND 07:51:13.49 -28:42:33.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 157555_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
Preparing report for the candidate 157555_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
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Considering the candidate 157592_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 157592_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
**** FOUND 07:56:07.49 -30:53:44.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 157595_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 157595_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
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Considering the candidate 157597_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 157597_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
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Considering the candidate 157629_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 157629_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
**** FOUND 08:02:25.29 -32:30:59.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 157634_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 157634_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
**** FOUND 08:38:43.98 -34:33:18.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 157699_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 157699_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
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Considering the candidate 157769_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
Preparing report for the candidate 157769_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
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Considering the candidate 157849_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
Preparing report for the candidate 157849_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
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Considering the candidate 157874_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 157874_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
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Considering the candidate 157875_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 157875_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
**** FOUND 07:56:44.76 -29:21:23.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 157879_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
Preparing report for the candidate 157879_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
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Considering the candidate 157999_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 157999_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
**** FOUND 07:48:37.32 -33:40:12.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 158002_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 158002_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
**** FOUND 08:10:02.58 -33:08:29.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 158004_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 158004_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
**** FOUND 08:43:41.32 -37:19:40.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 158011_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 158011_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
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Considering the candidate 158028_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 158028_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
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Considering the candidate 158035_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 158035_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
**** FOUND 07:56:25.21 -36:56:59.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 158050_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 158050_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
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Considering the candidate 158102_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 158102_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
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Considering the candidate 158143_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
Preparing report for the candidate 158143_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
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Considering the candidate 158145_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 158145_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
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Considering the candidate 158156_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 158156_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
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Considering the candidate 158180_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 158180_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
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Considering the candidate 158202_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 158202_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
Rejecting candidate due to large distance (28.8") between the two second-epoch detections
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Considering the candidate 158210_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 158210_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
**** FOUND 08:26:18.67 -29:35:53.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 158224_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 158224_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
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Considering the candidate 158241_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 158241_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
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Considering the candidate 158244_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 158244_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
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Considering the candidate 158249_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 158249_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
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Considering the candidate 158264_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 158264_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
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Considering the candidate 158285_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 158285_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
Rejecting candidate due to large distance (28.6") between the two second-epoch detections
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Considering the candidate 158293_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 158293_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
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Considering the candidate 158304_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 158304_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
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Considering the candidate 158327_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 158327_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
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Considering the candidate 158331_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 158331_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 158335_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 158335_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
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Considering the candidate 158341_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 158341_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
**** FOUND 08:03:34.61 -34:20:52.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 158370_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 158370_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 158377_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 158377_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 158397_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 158397_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 158402_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 158402_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 158410_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 158410_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
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Considering the candidate 158429_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 158429_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
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Considering the candidate 158436_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 158436_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
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Considering the candidate 158458_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 158458_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
**** FOUND 08:17:45.42 -29:53:46.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 158474_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 158474_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
Rejecting candidate due to large distance (29.5") between the two second-epoch detections
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Considering the candidate 158526_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
Preparing report for the candidate 158526_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
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Considering the candidate 158557_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
Preparing report for the candidate 158557_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 142862_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
Preparing report for the candidate 142862_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 143439_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
Preparing report for the candidate 143439_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 55630_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
Preparing report for the candidate 55630_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 30394_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
Preparing report for the candidate 30394_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04288_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
Preparing report for the candidate 04288_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 110176_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 110176_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
**** FOUND 08:02:43.86 -29:57:53.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 37293_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
Preparing report for the candidate 37293_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 91172_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 91172_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
**** FOUND 08:26:04.27 -30:06:41.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 146747_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 146747_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
**** FOUND 08:04:55.21 -30:20:56.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 112435_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 112435_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
**** FOUND 08:43:19.32 -29:56:56.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 144737_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 144737_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
**** FOUND 08:53:32.83 -34:18:59.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 143468_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 143468_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
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Considering the candidate 14083_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
Preparing report for the candidate 14083_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
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Considering the candidate 89944_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
Preparing report for the candidate 89944_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
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Considering the candidate 59166_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
Preparing report for the candidate 59166_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 61578_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 61578_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
**** FOUND 08:43:12.00 -33:05:46.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 78633_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
Preparing report for the candidate 78633_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 91132_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 91132_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
**** FOUND 08:12:30.55 -30:09:04.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 25519_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
Preparing report for the candidate 25519_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14890_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
Preparing report for the candidate 14890_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16183_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 16183_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
**** FOUND 08:51:34.68 -36:43:59.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 09348_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 09348_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 67959_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
Preparing report for the candidate 67959_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13072_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 13072_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
**** FOUND 08:08:56.51 -37:28:14.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 127206_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 127206_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
**** FOUND 08:18:45.59 -31:51:12.0 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 02313_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
Preparing report for the candidate 02313_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72099_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 72099_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
**** FOUND 08:07:03.60 -32:38:45.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10979_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
Preparing report for the candidate 10979_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24487_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 24487_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
**** FOUND 08:02:05.74 -36:17:08.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 25062_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
Preparing report for the candidate 25062_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16623_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 16623_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68587_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 68587_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
**** FOUND 07:49:30.66 -32:43:10.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 09320_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
Preparing report for the candidate 09320_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 28995_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 28995_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33734_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 33734_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
**** FOUND 08:23:19.18 -35:24:59.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23909_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 23909_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
**** FOUND 08:42:49.86 -36:08:34.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 70514_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 70514_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
**** FOUND 08:43:40.94 -32:31:39.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19210_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
Preparing report for the candidate 19210_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35555_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 35555_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
**** FOUND 08:04:27.18 -35:15:12.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02345_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 02345_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
**** FOUND 08:23:04.28 -38:48:29.2 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06745_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456
The candidate 06745_fd_Pup-04-Q1b1x1_2026-11-03_03-45-02_20.00sec_-0.00C_LIGHTs_0456 did not pass the final checks
**** FOUND 08:09:40.01 -38:10:28.7 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 2s
make_report_in_HTML.sh TOTAL: 80s
Prepared the HTML report for the field Pup-04-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
08:23:04.30 -38:48:29.5
08:18:45.59 -31:51:11.9
08:13:51.85 -38:54:58.3
08:03:52.56 -38:36:11.0
08:38:22.51 -37:45:13.3
08:26:59.23 -37:39:52.0
08:19:39.08 -37:20:06.6
08:25:48.37 -36:57:08.8
08:04:18.60 -36:22:27.1
08:19:08.23 -37:14:32.8
08:18:37.68 -33:38:10.7
08:24:42.77 -32:26:53.0
07:52:16.86 -32:23:16.5
08:29:24.56 -35:29:56.3
07:57:56.45 -30:22:00.0
08:12:41.18 -34:04:59.7
08:18:50.99 -35:13:48.8
08:20:10.46 -35:16:42.2
08:50:35.40 -36:27:09.6
08:19:40.15 -36:15:03.6
08:40:16.69 -36:02:10.9
08:42:35.92 -35:31:42.5
08:29:03.43 -35:04:07.1
08:11:13.06 -33:45:06.2
07:58:41.43 -33:26:43.2
07:58:56.11 -32:51:56.9
08:24:53.86 -32:10:06.0
08:48:37.59 -29:33:44.5
########### Completed Pup-04-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
08:18:45.59 -31:51:11.9
08:23:04.30 -38:48:29.5
08:18:37.68 -33:38:10.7
08:24:42.77 -32:26:53.0
07:52:16.86 -32:23:16.5
08:29:24.56 -35:29:56.3
07:57:56.45 -30:22:00.0
08:12:41.18 -34:04:59.7
08:18:50.99 -35:13:48.8
08:20:10.46 -35:16:42.2
08:25:48.37 -36:57:08.8
08:04:18.60 -36:22:27.1
08:11:13.06 -33:45:06.2
08:42:35.92 -35:31:42.5
08:03:52.56 -38:36:11.0
08:29:03.43 -35:04:07.1
08:19:39.08 -37:20:06.6
08:48:37.59 -29:33:44.5
07:58:41.43 -33:26:43.2
08:24:53.86 -32:10:06.0
08:40:16.69 -36:02:10.9
08:19:08.23 -37:14:32.8
07:58:56.11 -32:51:56.9
08:13:51.85 -38:54:58.3
08:26:59.23 -37:39:52.0
08:19:40.15 -36:15:03.6
08:38:22.51 -37:45:13.3
08:50:35.40 -36:27:09.6
###################################################################################
08:18:45.59 -31:51:11.9 -- not an asteroid (will add it to exclusion list)
08:23:04.30 -38:48:29.5 -- not an asteroid (will add it to exclusion list)
08:18:37.68 -33:38:10.7 -- not an asteroid (will add it to exclusion list)
08:24:42.77 -32:26:53.0 -- not an asteroid (will add it to exclusion list)
07:52:16.86 -32:23:16.5 -- not an asteroid (will add it to exclusion list)
08:29:24.56 -35:29:56.3 -- not an asteroid (will add it to exclusion list)
07:57:56.45 -30:22:00.0 -- not an asteroid (will add it to exclusion list)
08:12:41.18 -34:04:59.7 -- not an asteroid (will add it to exclusion list)
08:18:50.99 -35:13:48.8 -- not an asteroid (will add it to exclusion list)
08:20:10.46 -35:16:42.2 -- not an asteroid (will add it to exclusion list)
08:25:48.37 -36:57:08.8 -- not an asteroid (will add it to exclusion list)
08:04:18.60 -36:22:27.1 -- not an asteroid (will add it to exclusion list)
08:11:13.06 -33:45:06.2 -- not an asteroid (will add it to exclusion list)
08:42:35.92 -35:31:42.5 -- not an asteroid (will add it to exclusion list)
08:03:52.56 -38:36:11.0 -- not an asteroid (will add it to exclusion list)
08:29:03.43 -35:04:07.1 -- not an asteroid (will add it to exclusion list)
08:19:39.08 -37:20:06.6 -- not an asteroid (will add it to exclusion list)
08:48:37.59 -29:33:44.5 -- not an asteroid (will add it to exclusion list)
07:58:41.43 -33:26:43.2 -- not an asteroid (will add it to exclusion list)
08:24:53.86 -32:10:06.0 -- not an asteroid (will add it to exclusion list)
08:40:16.69 -36:02:10.9 -- not an asteroid (will add it to exclusion list)
08:19:08.23 -37:14:32.8 -- not an asteroid (will add it to exclusion list)
07:58:56.11 -32:51:56.9 -- not an asteroid (will add it to exclusion list)
08:13:51.85 -38:54:58.3 -- not an asteroid (will add it to exclusion list)
08:26:59.23 -37:39:52.0 -- not an asteroid (will add it to exclusion list)
08:19:40.15 -36:15:03.6 -- not an asteroid (will add it to exclusion list)
08:38:22.51 -37:45:13.3 -- not an asteroid (will add it to exclusion list)
08:50:35.40 -36:27:09.6 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
07:52:16.86 -32:23:16.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:57:56.45 -30:22:00.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:58:41.43 -33:26:43.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:58:56.11 -32:51:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
08:03:52.56 -38:36:11.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:04:18.60 -36:22:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:11:13.06 -33:45:06.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:12:41.18 -34:04:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
08:13:51.85 -38:54:58.3 -- does not seem to be a hot pixel (will add it to exclusion list)
08:18:37.68 -33:38:10.7 -- does not seem to be a hot pixel (will add it to exclusion list)
08:18:45.59 -31:51:11.9 -- does not seem to be a hot pixel (will add it to exclusion list)
08:18:50.99 -35:13:48.8 -- does not seem to be a hot pixel (will add it to exclusion list)
08:19:08.23 -37:14:32.8 -- does not seem to be a hot pixel (will add it to exclusion list)
08:19:39.08 -37:20:06.6 -- does not seem to be a hot pixel (will add it to exclusion list)
08:19:40.15 -36:15:03.6 -- does not seem to be a hot pixel (will add it to exclusion list)
08:20:10.46 -35:16:42.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:23:04.30 -38:48:29.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:24:42.77 -32:26:53.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:24:53.86 -32:10:06.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:25:48.37 -36:57:08.8 -- does not seem to be a hot pixel (will add it to exclusion list)
08:26:59.23 -37:39:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:29:03.43 -35:04:07.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:29:24.56 -35:29:56.3 -- does not seem to be a hot pixel (will add it to exclusion list)
08:38:22.51 -37:45:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
08:40:16.69 -36:02:10.9 -- does not seem to be a hot pixel (will add it to exclusion list)
08:42:35.92 -35:31:42.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:48:37.59 -29:33:44.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:50:35.40 -36:27:09.6 -- 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)
07:52:16.86 -32:23:16.5 -- a known variable star
07:57:56.45 -30:22:00.0 -- a known variable star
07:58:41.43 -33:26:43.2 -- a known variable star
07:58:56.11 -32:51:56.9 -- a known variable star
08:03:52.56 -38:36:11.0 -- a known variable star
08:04:18.60 -36:22:27.1 -- a known variable star
08:11:13.06 -33:45:06.2 -- a known variable star
08:12:41.18 -34:04:59.7 -- a known variable star
08:13:51.85 -38:54:58.3 -- a known variable star
08:18:37.68 -33:38:10.7 -- a known variable star
08:18:45.59 -31:51:11.9 -- a known variable star
08:18:50.99 -35:13:48.8 -- a known variable star
08:19:08.23 -37:14:32.8 -- a known variable star
08:19:39.08 -37:20:06.6 -- a known variable star
08:19:40.15 -36:15:03.6 -- a known variable star
08:20:10.46 -35:16:42.2 -- a known variable star
08:23:04.30 -38:48:29.5 -- a known variable star
08:24:42.77 -32:26:53.0 -- a known variable star
08:24:53.86 -32:10:06.0 -- a known variable star
08:25:48.37 -36:57:08.8 -- a known variable star
08:26:59.23 -37:39:52.0 -- a known variable star
08:29:03.43 -35:04:07.1 -- a known variable star
08:29:24.56 -35:29:56.3 -- a known variable star
08:38:22.51 -37:45:13.3 -- a known variable star
08:40:16.69 -36:02:10.9 -- a known variable star
08:42:35.92 -35:31:42.5 -- a known variable star
08:48:37.59 -29:33:44.5 -- a known variable star
08:50:35.40 -36:27:09.6 -- a known variable star
Found 0 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
28 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
###################################################################################
exclusion_list_gaiadr2.txt NOT FOUND
exclusion_list_apass.txt NOT FOUND
IS_THIS_TEST_RUN= NO ALLOW_EXCLUSION_LIST_UPDATE= YES
#### Adding the following to the exclusion list ####
07:52:16.86 -32:23:16.5
07:57:56.45 -30:22:00.0
07:58:41.43 -33:26:43.2
07:58:56.11 -32:51:56.9
08:03:52.56 -38:36:11.0
08:04:18.60 -36:22:27.1
08:11:13.06 -33:45:06.2
08:12:41.18 -34:04:59.7
08:13:51.85 -38:54:58.3
08:18:37.68 -33:38:10.7
08:18:45.59 -31:51:11.9
08:18:50.99 -35:13:48.8
08:19:08.23 -37:14:32.8
08:19:39.08 -37:20:06.6
08:19:40.15 -36:15:03.6
08:20:10.46 -35:16:42.2
08:23:04.30 -38:48:29.5
08:24:42.77 -32:26:53.0
08:24:53.86 -32:10:06.0
08:25:48.37 -36:57:08.8
08:26:59.23 -37:39:52.0
08:29:03.43 -35:04:07.1
08:29:24.56 -35:29:56.3
08:38:22.51 -37:45:13.3
08:40:16.69 -36:02:10.9
08:42:35.92 -35:31:42.5
08:48:37.59 -29:33:44.5
08:50:35.40 -36:27:09.6
####################################################
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461347.90581687 -observatory V36
14:42:39.66 -16:35:39.9 Mercury (5.4mag)
13:25:21.12 -13:34:07.8 Venus (-4.3mag)
09:29:37.11 +16:33:11.0 Mars (0.8mag)
09:47:06.32 +14:06:04.8 Jupiter (-2.0mag)
00:36:24.70 +01:00:34.3 Saturn (0.5mag)
04:09:01.60 +20:50:07.3 Uranus (5.6mag)
00:08:19.87 -00:38:17.7 Neptune (7.7mag)
20:24:28.42 -23:41:32.4 Pluto (14.5mag)
10:12:17.31 +10:34:54.9 Moon (-9.8mag)
-rw-r--r-- 1 apache apache 361 Nov 3 03:52 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461347.90581687:
09:47:00.20 +14:06:40.6 Io (6.0mag)
09:46:58.04 +14:06:54.0 Europa (6.1mag)
09:47:19.29 +14:04:50.5 Ganymede (5.5mag)
09:47:35.87 +14:03:16.4 Callisto (6.8mag)
09:48:33.44 +14:15:34.0 Himalia (15.5mag)
09:47:04.26 +14:06:17.1 Thebe (16.3mag)
09:46:52.38 +14:31:05.6 Elara (17.4mag)
09:47:51.74 +13:33:45.4 Pasiphae (17.7mag)
09:44:07.82 +14:37:59.7 Carme (18.7mag)
00:36:33.66 +01:00:06.0 Titan (8.3mag)
00:36:25.21 +01:00:35.5 Rhea (9.6mag)
00:36:55.07 +01:01:13.3 Iapetus (11.0mag)
00:36:13.53 +01:00:14.4 Hyperion (14.2mag)
00:34:37.97 +00:48:24.8 Phoebe (16.4mag)
-rw-r--r-- 1 apache apache 568 Nov 3 03:53 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461347.90581687:
04:35:21.03 +17:21:24.7 JWST
15:04:09.20 +53:29:49.4 Chandra
07:10:56.17 -13:54:31.5 XMM-Newton
-rw-r--r-- 1 apache apache 96 Nov 3 03:52 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461347.90581687 -observatory V36
03:33:39.20 +19:56:50.1 17.1mag P/1996 R2 (Lagerkvist)
07:46:38.02 +38:23:03.8 17.9mag P/2004 V5 (LINEAR-Hill)
07:46:43.38 +38:22:50.8 17.9mag P/2004 V5-A (LINEAR-Hill)
07:46:01.93 +38:23:10.5 17.9mag P/2004 V5-B (LINEAR-Hill)
05:01:54.57 +39:06:41.6 17.8mag P/2009 Y2 (Kowalski)
18:48:04.33 -32:52:38.8 15.0mag P/2010 H2 (Vales)
07:45:18.09 -73:54:21.1 17.2mag C/2014 UN271 (Bernardinelli-Bernstein)
06:11:29.02 +35:18:30.8 17.7mag C/2017 K2 (PANSTARRS)
07:35:42.74 +25:20:22.3 16.9mag C/2022 N2 (PANSTARRS)
09:08:34.40 +38:31:48.8 16.4mag C/2024 E1 (Wierzchos)
18:37:00.38 +40:52:18.1 17.4mag C/2024 J3 (ATLAS)
05:43:03.70 -13:33:18.7 16.3mag C/2024 T5 (ATLAS)
14:15:16.14 -04:35:14.0 16.3mag C/2025 Y1 (ATLAS)
20:14:44.71 +53:05:24.0 15.2mag C/2026 A2 (Bok)
13:07:35.14 +16:59:06.9 17.7mag A/2026 E1
16:00:37.96 -65:25:15.5 14.5mag P/2026 R2 (Leonard)
19:34:03.72 -05:22:09.4 17.1mag P/2026 T1 (ATLAS)
23:28:54.94 +14:03:37.0 16.8mag 2P/Encke
23:26:03.28 -25:46:41.4 15.4mag 10P/Tempel
02:39:55.87 +30:34:29.0 16.3mag 11P/Tempel-Swift-LINEAR
12:26:09.42 -10:02:08.1 16.3mag 29P/Schwassmann-Wachmann
00:10:40.91 -09:01:22.6 15.9mag 65P/Gunn
08:00:12.01 +13:35:14.3 14.0mag 78P/Gehrels
08:59:46.78 +45:56:58.6 17.1mag 112P/Urata-Niijima
09:51:08.01 +05:35:51.9 17.8mag 114P/Wiseman-Skiff
12:26:52.61 +08:02:51.4 14.8mag 123P/West-Hartley
19:48:57.62 +14:24:39.9 10.2mag 161P/Hartley-IRAS
11:12:09.63 -03:06:22.6 16.2mag 169P/NEAT
09:41:34.47 +23:29:53.0 18.0mag 186P/Garradd
03:10:42.16 +02:11:19.3 15.3mag 220P/McNaught
06:22:38.79 +49:46:08.4 15.6mag 260P/McNaught
07:56:28.63 +25:04:34.1 17.6mag 266P/Christensen
-rw-r--r-- 1 apache apache 1.6K Nov 3 03:52 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
17:54:18.84 -27:36:35.70 TCP J17541876-2736362 2026-10-24.76 9.92
10:38:47.97 +53:30:34.00 SN2026sqf 2026-10-24.6 13.27
21:49:53.30 +14:07:44.90 ASASSN-26fq 2026-10-23.23 14.82
01:00:14.36 +34:04:05.90 ASASSN-26fp 2026-10-23.34 12.9
01:06:23.14 -63:46:37.10 ASASSN-26fo 2026-10-19.79 -4.88
00:25:28.03 +20:14:39.10 SN2026afqd 2026-10-19.36 -0.77
22:14:03.37 -45:07:18.60 ASASSN-26fm 2026-10-13.75 14.42
01:57:48.19 -33:14:42.30 SN 2026aedl 2026-10-12.33 15.3
18:05:22.06 +17:52:41.00 ASASSN-26fn 2026-10-11.74 15.23
21:50:55.86 -02:51:49.30 SN2026acyb 2026-10-9.85 16.83
03:40:34.04 +02:31:56.70 SN2026acvp 2026-10-9.95 17.75
04:33:25.91 -13:41:04.20 SN2026adhl 2026-10-9.94 17.52
09:20:05.05 +27:03:12.40 SN2026aeif 2026-10-9.47 15.93
02:58:07.77 -65:18:52.90 ASASSN-26fl 2026-10-7.9 -0.85
02:49:03.98 -49:55:57.00 SN 2026adfy 2026-10-4.88 16.61
22:03:46.31 -11:07:57.70 AT2026adgn 2026-10-4.28 -2.56
15:03:12.98 +49:51:05.40 ASASSN-26fj 2026-10-2.06 15.91
08:07:27.96 -65:51:03.90 ASASSN-26fi 2026-10-1.36 15.82
21:02:34.66 +23:57:26.20 ASASSN-26fh 2026-10-1.27 15.94
20:00:16.62 +03:26:29.90 AT2026adfv 2026-10-1.3 16.42
00:08:42.74 -32:33:16.50 SN2026abhc 2026-09-29.15 15.57
21:02:30.26 -19:27:41.80 SN2026acxa 2026-09-29.13 14.65
04:39:17.45 -28:06:12.40 ASASSN-26fg 2026-09-23.25 15.73
05:25:07.80 +04:38:32.40 SN2026aajs 2026-09-21.32 17.04
19:56:12.67 +08:25:27.70 AT2026acgs 2026-09-18.14 15.84
00:02:34.06 +52:55:18.90 ASASSN-26ff 2026-09-16.38 15.41
23:44:33.18 +17:46:12.20 SN2026yjv 2026-09-15.38 18.32
16:21:12.24 +57:37:51.30 SN 2026aafh 2026-09-14.11 15.02
23:36:00.27 -19:28:18.00 SN 2026aaks 2026-09-14.44 16.89
16:35:24.86 -05:32:38.20 SN2026aasi 2026-09-12.99 16.58
16:46:08.71 +37:25:21.80 SN2026aafk 2026-09-13.25 17.4
23:48:37.86 +50:25:24.60 SN2026aafs 2026-09-13.47 17
21:20:27.02 +02:10:42.50 SN2026aagh -------
08:02:26.85 -24:37:44.10 ASASSN-26fe 2026-09-13.34 13.67
02:29:34.91 +23:06:56.30 SN2026aars 2026-09-12.27 16.93
02:47:25.52 -32:58:34.50 SN 2026znh 2026-09-9.92 16.26
04:59:14.53 -83:27:58.80 ASASSN-26fd 2026-09-9.11 17.27
17:52:06.79 -23:43:20.70 ASASSN-26fc 2026-09-8.79 12.14
03:52:53.26 -14:19:28.70 SN 2026zfw 2026-09-8 17.78
01:53:26.46 +10:07:25.10 SN2026aacj 2026-09-7.17 16.27
20:04:34.47 +62:38:38.10 SN2026zji 2026-09-7.14 15.87
22:37:05.64 +34:24:35.00 SN2026aaiv 2026-09-7.25 13.48
22:24:21.29 -10:25:31.60 ASASSN-26fb 2026-09-5.3 13.93
00:44:54.28 +41:33:10.50 AT2026aabo 2026-09-3.29 15.02
00:52:12.40 -58:22:08.60 SN 2026zhl 2026-08-31.92 16.51
19:53:57.87 +61:00:19.70 ASASSN-26fa 2026-08-31.18 14.63
00:21:50.96 -09:29:16.30 AT2026zwp 2026-08-31.41 15.59
19:45:06.20 +18:22:48.80 V488 2026-08-30.13 9.37
18:25:12.79 -22:25:29.10 V8055 2026-08-30 10.76
17:17:45.96 +64:31:40.10 ASASSN-26ez 2026-08-25.13 10.87
19:02:47.09 +58:08:21.00 AT2026zwo 2026-08-24.16 15.78
04:20:07.58 -42:26:59.90 AT2026zjy 2026-08-23.03 15.91
03:08:18.02 +11:54:46.50 SN2026ymb 2026-08-23.4 16.44
20:22:32.48 -50:45:14.30 SN2026yid 2026-08-22.82 15.13
04:24:28.39 -56:20:21.60 ASASSN-26ey 2026-08-20.02 15.55
16:46:37.81 -63:14:59.80 ASASSN-26ex 2026-08-18.78 3.63
21:28:47.85 +20:31:03.60 SN 2026sfn 2026-08-16.3 17.09
23:01:28.67 -61:00:39.00 SN 2026yib 2026-08-14.85 17.36
00:22:23.20 -32:16:02.70 SN 2026whu 2026-08-14.96 16.5
19:56:21.71 -37:24:19.90 ASASSN-26ew 2026-08-13.82 14.73
13:53:14.21 +00:26:52.00 SN 2026wkv 2026-08-10.12 15.83
05:21:07.61 +23:38:20.10 TCP J05210763+2338194 2026-08-10.59 9.34
01:28:20.49 +40:13:27.10 SN2026wpd 2026-08-9.34 16.37
23:47:50.87 +49:28:49.80 SN2026wjs 2026-08-9.35 17.12
16:03:20.92 +17:43:23.70 AT2026xau 2026-08-9.3 17.71
01:10:22.05 -09:34:08.50 SN2026weo 2026-08-7.46 15.76
00:56:54.35 -35:55:29.40 AT2026wdy 2026-08-5.05 16.08
22:08:07.63 -53:03:58.90 AT2026wek 2026-08-3.82 17.17
14:51:51.34 +66:13:24.60 ASASSN-26ev 2026-08-2.15 14.02
12:06:50.79 -36:16:06.20 SN2026wgm 2026-08-1.73 15.61
16:56:36.90 -59:29:26.00 ASASSN-26er 2026-07-25.82 15.09
01:21:27.89 -10:37:05.90 SN2026vbh 2026-07-25.05 15.79
21:17:31.59 +22:25:50.90 ASASSN-26eq 2026-07-24.37 15.13
18:53:36.89 +16:56:43.60 ASASSN-26ep 2026-07-23.47 -4.06
12:18:47.98 -30:48:47.50 ASASSN-26et 2026-07-22.76 13.98
13:00:47.82 +15:42:17.60 SN2026uwk 2026-07-21.75 16.38
18:52:31.11 -32:28:00.90 ASASSN-26en 2026-07-21.77 14.63
14:42:58.01 -62:32:59.10 ASASSN-26es 2026-07-20.79 15.36
20:12:45.57 -32:53:13.00 ASASSN-26em 2026-07-20.94 16.83
18:54:24.33 -46:11:51.70 ASASSN-26eu 2026-07-20.93 14.86
03:18:56.99 -80:55:10.40 AT2026ugi 2026-07-20.03 17.12
18:43:58.40 +24:22:41.80 ASASSN-26eo 2026-07-19.36 16.16
04:50:01.03 -02:22:33.80 ASASSN-26ej 2026-07-16.17 17.02
18:34:55.28 -31:41:00.90 ASASSN-26ek 2026-07-16.24 15.73
17:07:43.61 -44:21:53.50 ASASSN-26el 2026-07-15.86 16.01
14:45:08.35 +24:13:12.30 ASASSN-26ei 2026-07-16.17 16.46
10:00:46.44 -32:36:31.10 AT 2023mhb 2026-07-14.73 16.67
14:39:37.45 -11:22:36.20 AT 2026unl 2026-07-15.27 17.11
10:49:42.57 -11:25:55.80 ASASSN-26eh 2026-07-14.72 16.58
19:33:53.06 -07:15:00.80 ASASSN-22le 2026-07-14.15 15.5
02:45:40.52 -27:55:30.30 ASASSN-26ef 2026-07-12.35 15.86
23:26:43.80 +04:42:39.70 SN 2026qtn 2026-07-12.22 16.47
02:19:17.26 +28:57:15.40 ASASSN-26ec 2026-07-11.53 2.78
18:31:15.56 -05:34:31.50 AT2026stb 2026-07-11.28 -1.29
13:36:08.24 +23:29:05.00 AT2026pjf 2026-07-10.18 -0.72
17:33:39.82 +04:22:36.70 SN2026pir 2026-07-9.86 -0.66
11:21:41.26 -50:33:36.30 ASASSN-26ed 2026-07-8.8 -1.3
23:41:42.11 +26:29:49.10 AT2026qil 2026-07-9.3 16.15
20:21:30.50 -32:03:40.10 ASASSN-26ee 2026-07-7.22 15.53
19:37:44.09 -05:35:42.80 AT2026ryu 2026-07-7.17 14.88
-rw-r--r-- 1 apache apache 5.7K Nov 3 03:52 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
19:45:06.48 +18:22:42.2 PNV J19450648+1822422 2026-08-25.1278 9.0mag
00:42:54.65 +41:22:59.3 PNV J00425465+4122593 2026-08-25.4712 18.9mag
00:42:50.38 +41:18:58.76 PNV J00425038+4118587 2026-09-04.1512 18.2mag
00:42:12.76 +41:16:28.4 PNV J00421276+4116284 2026-09-10.9176 18.67Cmag
17:52:06.80 -23:43:20.7 TCP J17520680-2343207 2026-09-08.7896 12.6mag
00:42:40.94 +41:15:37.1 PNV J00424094+4115371 2026-09-17.8925 18.3mag
08:49:20.13 -09:19:15.8 TCP J08492013-0919158 2026-09-18.4698 13.3mag
00:42:13.93 +41:16:35.6 PNV J00421393+4116356 2026-09-22.6597 19.66Cmag
18:14:01.58 +15:13:55.5 TCP J18140158+1513555 2026-09-24.4645 14.1mag
00:42:36.61 +41:13:50.5 TCP J00423661+4113505 2026-09-29.7462 17.4mag
22:03:46.29 -11:07:57.8 TCP J22034629-1107578 2026-09-29.7438 14.51Cmag
22:05:02.06 +20:49:01.2 TCP J22050206+2049012 2026-10-03.5715 17.13Cmag
00:38:15.01 +41:14:47.2 TCP J00381501+4114472 2026-10-08.5978 17.72Cmag
01:06:05.83 +09:51:20.4 TCP J01060583+0951204 2026-10-10.8543 14.54Cmag
17:54:18.76 -27:36:36.2 TCP J17541876-2736362 2026-10-12.3993 10.8mag
09:56:00.79 +69:06:15.2 PNV J09560079+6906152 2026-10-14.9274 19.38Cmag
00:43:30.83 +41:26:55.3 PNV J00433083+4126553 2026-10-17.5651 18.61Cmag
04:57:32.08 +30:15:41.6 TCP J04573208+3015416 2026-10-17.7818 18.21Cmag
05:21:07.64 +23:38:21.3 TCP J05210764+2338213 2026-10-18.4020 10.3mag
05:34:11.01 +28:45:30.5 TCP J05341101+2845305 2026-10-18.3604 16.6mag
-rw-r--r-- 1 apache apache 191K Nov 3 03:52 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
09:05:17.957 +16:54:24.18 AT 2026afqz 2026-10-14.48 20.4887
08:54:21.666 +09:12:48.44 AT 2026afqy 2026-10-14.49 20.3035
09:25:26.154 +14:49:42.05 SN 2026afqx 2026-09-24.53 19.3798
04:49:00.563 -20:22:30.78 AT 2026afqw 2026-10-16.48 19.4415
07:26:25.375 -34:28:52.68 AT 2026afqv 2026-10-17.34 19.271
21:46:13.715 +36:36:26.80 AT 2026afqu 2026-10-15.87 19.7
03:11:38.085 -02:01:36.09 AT 2026afqt 2026-10-16.06 19.51
07:41:25.037 +21:02:16.50 SN 2026afqs 2026-10-13.18 19.73
08:37:58.823 +12:32:25.90 SN 2026afqr 2026-10-17.23 19.93
04:51:17.403 -26:27:57.01 AT 2026afqq 2026-10-17.26 19.449
04:37:45.596 -24:04:12.02 AT 2026afqp 2026-10-17.26 19.535
01:25:03.389 -32:39:10.49 AT 2026afqo 2026-10-12.21 19.322
03:17:26.864 -15:58:34.85 AT 2026afqn 2026-10-17.30 19.375
17:53:52.220 +41:47:24.16 AT 2026afqm 2026-10-16.83 19.331
06:23:17.419 +70:33:15.10 SN 2026afql 2026-10-17.15 18.737
02:38:36.934 +41:55:58.84 SN 2026afqk 2026-10-17.04 19.369
05:26:14.588 -27:06:01.24 AT 2026afqj 2026-10-17.29 19.31
02:01:09.758 -36:18:14.69 AT 2026afqi 2026-10-12.26 19.361
09:44:49.328 +38:11:23.47 SN 2026afqh 2026-10-17.22 18.467
17:38:02.102 +55:52:14.30 AT 2026afqg 2026-10-16.84 19.253
-rw-r--r-- 1 apache apache 89K Nov 3 03:52 tns_transients_list.txt
