This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pyx-02-Q1b1x1_053531_TTUQ1b1x1_1550823_YDJ5pKlT
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 03.4820 2461347.9820 10.56 09:18:47.01 -35:44:18.1
261.71853 9.59989 galactic Pyx Second-epoch detections are separated by 0.9" and 7.6 pix
The object was found in VSX 0" ASAS J091847-3544.3
Type: MISC
# Max. Min./Amp. JD0 Period
12.430 V Y 1.000 V 2452537.00000 355.000000000000 S6*5
The object was not found in astcheck.
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:18:47.01 -35:44:18.1: 11.60 +/- 0.02 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:18:47.01 -35:44:18.1: 11.61 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.60 +/- 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
ASAS J091847-3544.3,2461347.9820,10.56,0.05,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 J091847-3544.3 20261103.4820 10.56CV 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 03.4820 2461347.9820 10.70 09:57:01.14 -35:57:42.2
267.68239 14.70562 galactic Ant Second-epoch detections are separated by 0.2" and 7.2 pix
The object was found in VSX 5" ASAS J095702-3557.7
Type: M
# Max. Min./Amp. JD0 Period
11.090 V Y 1.950 CV 2452590.50000 366.837857500000
The object was not found in astcheck.
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:57:01.14 -35:57:42.2: 13.08 +/- 0.12 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:57:01.14 -35:57:42.2: 13.04 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.06 +/- 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!
TCP 2026 11 03.4820* 09 57 01.14 -35 57 42.2 10.7 U Ant 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 J095702-3557.7,2461347.9820,10.70,0.05,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 J095702-3557.7 20261103.4820 10.70CV 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 03.4820 2461347.9820 10.08 09:17:02.79 -32:04:35.2
258.75662 11.85193 galactic Pyx Second-epoch detections are separated by 0.2" and 7.5 pix
The object was found in VSX 1" ASAS J091703-3204.6
Type: MISC
# Max. Min./Amp. JD0 Period
11.450 V Y 0.780 V 2452217.60000 78.500000000000
The object was not found in astcheck.
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:17:02.79 -32:04:35.2: 11.11 +/- 0.01 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:17:02.79 -32:04:35.2: 11.14 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.12 +/- 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
ASAS J091703-3204.6,2461347.9820,10.08,0.05,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 J091703-3204.6 20261103.4820 10.08CV 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 03.4820 2461347.9820 9.90 09:11:04.45 -33:35:11.2
259.02458 9.90651 galactic Pyx Second-epoch detections are separated by 0.4" and 7.6 pix
The object was found in VSX 0" ASAS J091105-3335.2
Type: MISC
# Max. Min./Amp. JD0 Period
10.930 V Y 0.440 V 2452262.80000 76.400000000000
The object was not found in astcheck.
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:11:04.45 -33:35:11.2: 10.94 +/- 0.01 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:11:04.45 -33:35:11.2: 10.95 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.95 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin 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 J091105-3335.2,2461347.9820,9.90,0.05,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
ASAS J091105-3335.2 20261103.4820 9.90CV 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 03.4820 2461347.9820 11.20 09:31:04.47 -38:12:21.4
265.24823 9.59366 galactic Ant Second-epoch detections are separated by 0.3" and 7.5 pix
The object was found in VSX 1" ASAS J093104-3812.4
Type: M
# Max. Min./Amp. JD0 Period
12.780 V Y 2.410 V 2452826.30000 283.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:31:04.47 -38:12:21.4: 14.12 +/- 0.22 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:31:04.47 -38:12:21.4: 14.67 +/- 0.34 detection
Forced photometry reference-image weighted average: 14.28 +/- 0.19
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 03.4820* 09 31 04.47 -38 12 21.4 11.2 U Ant 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 J093104-3812.4,2461347.9820,11.20,0.05,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
ASAS J093104-3812.4 20261103.4820 11.20CV 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 03.4820 2461347.9820 11.79 09:31:49.20 -32:26:34.9
261.25970 13.83510 galactic Ant Second-epoch detections are separated by 0.3" and 7.3 pix
The object was found in VSX 3" CG Ant
Type: M
# Max. Min./Amp. JD0 Period
13.000 V < 14.800 V 2454766.00000 323.300000000000
The object was not found in astcheck.
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:31:49.20 -32:26:34.9: 14.52 +/- 0.27 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:31:49.20 -32:26:34.9: 14.84 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.52 +/- 0.27
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 03.4820* 09 31 49.20 -32 26 34.9 11.8 U Ant 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
CG Ant,2461347.9820,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
CG Ant 20261103.4820 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 03.4820 2461347.9820 12.04 09:29:37.12 -36:29:06.3
263.82159 10.62929 galactic Ant Second-epoch detections are separated by 1.1" and 7.5 pix
The object was found in VSX 1" ASAS J092937-3629.1
Type: MISC
# Max. Min./Amp. JD0 Period
9.471 Ic Y 0.639 Ic 2452892.50000 305.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:29:37.12 -36:29:06.3: 13.66 +/- 0.13 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:29:37.12 -36:29:06.3: 13.98 +/- 0.17 detection
Forced photometry reference-image weighted average: 13.78 +/- 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!
TCP 2026 11 03.4820* 09 29 37.12 -36 29 06.3 12.0 U Ant 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 J092937-3629.1,2461347.9820,12.04,0.05,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
ASAS J092937-3629.1 20261103.4820 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 03.4820 2461347.9820 12.31 09:04:28.37 -36:51:09.0
260.57491 6.72359 galactic Pyx Second-epoch detections are separated by 0.2" and 7.7 pix
The object was found in VSX 4" NSV 18131
Type: M:
# Max. Min./Amp. JD0 Period
14.200 P M
The object was not found in astcheck.
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:04:28.37 -36:51:09.0: 14.02 +/- 0.19 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:04:28.37 -36:51:09.0: 14.43 +/- 0.28 detection
Forced photometry reference-image weighted average: 14.15 +/- 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
NSV 18131,2461347.9820,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSV 18131 20261103.4820 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 03.4820 2461347.9820 12.54 09:17:03.27 -39:03:15.6
263.89819 7.05763 galactic Vel Second-epoch detections are separated by 3.0" and 7.2 pix
The object was found in VSX 3" ASASSN-V J091703.27-390318.3
Type: L
# Max. Min./Amp. JD0 Period
13.770 V 14.930 V
The object was not found in astcheck.
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:17:03.27 -39:03:15.6: 13.54 +/- 0.13 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:17:03.27 -39:03:15.6: 13.52 +/- 0.13 detection
Forced photometry reference-image weighted average: 13.53 +/- 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!
TCP 2026 11 03.4820* 09 17 03.27 -39 03 15.6 12.5 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
ASASSN-V J091703.27-390318.3,2461347.9820,12.54,0.05,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 J091703.27-390318.3 20261103.4820 12.54CV 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 03.4820 2461347.9820 12.96 09:28:56.61 -38:06:06.3
264.86937 9.37751 galactic Ant Second-epoch detections are separated by 0.7" and 7.4 pix
The object was found in VSX 1" ASASSN-V J092856.62-380607.0
Type: L
# Max. Min./Amp. JD0 Period
14.180 V 14.690 V
The object was not found in astcheck.
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:28:56.61 -38:06:06.3: 13.95 +/- 0.20 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:28:56.61 -38:06:06.3: 14.53 +/- 0.32 detection
Forced photometry reference-image weighted average: 14.11 +/- 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!
TCP 2026 11 03.4820* 09 28 56.61 -38 06 06.3 13.0 U Ant 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J092856.62-380607.0,2461347.9820,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J092856.62-380607.0 20261103.4820 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 03.4820 2461347.9820 13.00 09:23:45.46 -34:37:21.0
261.62288 11.10630 galactic Pyx Second-epoch detections are separated by 0.8" and 7.6 pix
The object was found in VSX 1" ASASSN-V J092345.42-343720.1
Type: L
# Max. Min./Amp. JD0 Period
14.600 V 15.140 V
The object was not found in astcheck.
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:23:45.46 -34:37:21.0: 14.75 +/- 0.33 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:23:45.46 -34:37:21.0: 14.22 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.36 +/- 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
ASASSN-V J092345.42-343720.1,2461347.9820,13.00,0.05,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
ASASSN-V J092345.42-343720.1 20261103.4820 13.00CV 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 03.4820 2461347.9820 12.98 09:52:12.34 -35:36:34.1
266.67518 14.35023 galactic Ant Second-epoch detections are separated by 3.0" and 7.2 pix
The object was found in VSX 3" ASASSN-V J095212.48-353632.0
Type: SR
# Max. Min./Amp. JD0 Period
14.100 V 16.000 V 2457821.80000 259.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:52:12.34 -35:36:34.1: 14.63 +/- 99.00 upperlimit
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:52:12.34 -35:36:34.1: 14.69 +/- 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!
TCP 2026 11 03.4820* 09 52 12.34 -35 36 34.1 13.0 U Ant 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J095212.48-353632.0,2461347.9820,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J095212.48-353632.0 20261103.4820 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 03.4820 2461347.9820 13.04 08:57:58.51 -35:50:25.1
258.94262 6.39701 galactic Pyx Second-epoch detections are separated by 1.0" and 7.6 pix
The object was found in VSX 9" ASASSN-V J085758.17-355016.6
Type: YSO
# Max. Min./Amp. JD0 Period
15.170 V 15.610 V
The object was not found in astcheck.
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 08:57:58.51 -35:50:25.1: 14.26 +/- 0.22 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 08:57:58.51 -35:50:25.1: 14.24 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.25 +/- 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
ASASSN-V J085758.17-355016.6,2461347.9820,13.04,0.05,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
ASASSN-V J085758.17-355016.6 20261103.4820 13.04CV 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 03.4820 2461347.9820 13.68 09:29:17.30 -29:41:41.1
258.85566 15.39580 galactic Ant Second-epoch detections are separated by 2.1" and 7.5 pix
The object was found in VSX 1" ASASSN-V J092917.40-294141.3
Type: SR
# Max. Min./Amp. JD0 Period
13.930 V 15.900 V 2457049.70000 193.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:29:17.30 -29:41:41.1: 14.65 +/- 0.28 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:29:17.30 -29:41:41.1: 14.96 +/- 0.36 detection
Forced photometry reference-image weighted average: 14.77 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 11 03.4820* 09 29 17.30 -29 41 41.1 13.7 U Ant 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J092917.40-294141.3,2461347.9820,13.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J092917.40-294141.3 20261103.4820 13.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 03.4820 2461347.9820 12.27 09:33:02.37 -38:52:40.4
266.00015 9.37206 galactic Ant Second-epoch detections are separated by 1.4" and 7.7 pix
The object was found in VSX 3" ASASSN-V J093302.51-385242.6
Type: L:
# Max. Min./Amp. JD0 Period
13.040 V 13.760 V
The object was not found in astcheck.
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:33:02.37 -38:52:40.4: 13.38 +/- 0.12 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:33:02.37 -38:52:40.4: 13.47 +/- 0.13 detection
Forced photometry reference-image weighted average: 13.43 +/- 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!
TCP 2026 11 03.4820* 09 33 02.37 -38 52 40.4 12.3 U Ant 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J093302.51-385242.6,2461347.9820,12.27,0.05,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 J093302.51-385242.6 20261103.4820 12.27CV 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 03.4820 2461347.9820 11.43 09:10:49.66 -37:24:12.8
261.84162 7.29575 galactic Vel Second-epoch detections are separated by 0.1" and 7.6 pix
The object was found in VSX 1" ASAS J091050-3724.2
Type: MISC
# Max. Min./Amp. JD0 Period
9.093 Ic Y 0.255 Ic 2452563.20000 68.990000000000 M7
The object was not found in astcheck.
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:10:49.66 -37:24:12.8: 12.36 +/- 0.04 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:10:49.66 -37:24:12.8: 12.42 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.39 +/- 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!
TCP 2026 11 03.4820* 09 10 49.66 -37 24 12.8 11.4 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 J091050-3724.2,2461347.9820,11.43,0.05,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 J091050-3724.2 20261103.4820 11.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 03.4820 2461347.9820 12.32 09:26:13.05 -32:18:16.1
260.29897 13.09648 galactic Pyx Second-epoch detections are separated by 0.6" and 7.3 pix
The object was found in VSX 1" ASASSN-V J092613.06-321814.9
Type: L
# Max. Min./Amp. JD0 Period
13.700 V 14.420 V
The object was not found in astcheck.
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:26:13.05 -32:18:16.1: 13.63 +/- 0.12 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:26:13.05 -32:18:16.1: 13.64 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.63 +/- 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
ASASSN-V J092613.06-321814.9,2461347.9820,12.32,0.05,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 J092613.06-321814.9 20261103.4820 12.32CV 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 03.4820 2461347.9820 11.55 09:20:59.40 -30:56:48.5
258.50202 13.23782 galactic Pyx Second-epoch detections are separated by 0.5" and 7.6 pix
The object was found in VSX 2" ASAS J092059-3056.8
Type: MISC
# Max. Min./Amp. JD0 Period
12.470 V Y 0.740 V 2452082.70000 186.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:20:59.40 -30:56:48.5: 12.51 +/- 0.04 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:20:59.40 -30:56:48.5: 12.69 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.59 +/- 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 J092059-3056.8,2461347.9820,11.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J092059-3056.8 20261103.4820 11.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 03.4820 2461347.9820 11.46 09:06:33.85 -37:11:06.4
261.10457 6.81444 galactic Pyx Second-epoch detections are separated by 0.9" and 7.8 pix
The object was found in VSX 1" ASAS J090634-3711.0
Type: MISC
# Max. Min./Amp. JD0 Period
12.950 V Y 0.920 V 2452013.10000 70.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:06:33.85 -37:11:06.4: 12.51 +/- 0.05 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:06:33.85 -37:11:06.4: 12.67 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.58 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin 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 J090634-3711.0,2461347.9820,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J090634-3711.0 20261103.4820 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 03.4820 2461347.9820 11.46 09:02:22.40 -37:09:34.4
260.52862 6.20605 galactic Pyx Second-epoch detections are separated by 0.5" and 7.6 pix
The object was found in VSX 1" DR Pyx
Type: SR
# Max. Min./Amp. JD0 Period
12.900 V < 14.200 V 220.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:02:22.40 -37:09:34.4: 12.46 +/- 0.04 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:02:22.40 -37:09:34.4: 12.61 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.53 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin 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
DR Pyx,2461347.9820,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DR Pyx 20261103.4820 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 03.4820 2461347.9820 11.44 09:39:17.59 -34:19:01.3
263.75319 13.55868 galactic Ant Second-epoch detections are separated by 0.7" and 7.5 pix
The object was found in VSX 2" ASAS J093918-3419.0
Type: MISC
# Max. Min./Amp. JD0 Period
8.918 Ic Y 0.401 Ic 2452777.60000 156.300000000000
The object was not found in astcheck.
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:39:17.59 -34:19:01.3: 12.47 +/- 0.05 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:39:17.59 -34:19:01.3: 12.48 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.48 +/- 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!
TCP 2026 11 03.4820* 09 39 17.59 -34 19 01.3 11.4 U Ant 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 J093918-3419.0,2461347.9820,11.44,0.05,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 J093918-3419.0 20261103.4820 11.44CV 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 03.4820 2461347.9820 11.22 09:31:23.67 -37:19:58.3
264.68059 10.26718 galactic Ant Second-epoch detections are separated by 1.0" and 7.5 pix
The object was found in VSX 2" ASAS J093124-3720.0
Type: MISC|EC
# Max. Min./Amp. JD0 Period
12.330 V Y 0.710 V 2452339.40000 136.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:31:23.67 -37:19:58.3: 12.43 +/- 0.04 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:31:23.67 -37:19:58.3: 12.51 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.47 +/- 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!
TCP 2026 11 03.4820* 09 31 23.67 -37 19 58.3 11.2 U Ant 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 J093124-3720.0,2461347.9820,11.22,0.05,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 J093124-3720.0 20261103.4820 11.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 03.4820 2461347.9820 11.47 09:31:53.73 -38:01:32.5
265.24010 9.83553 galactic Ant Second-epoch detections are separated by 1.0" and 7.2 pix
The object was found in VSX 1" ASAS J093154-3801.6
Type: MISC
# Max. Min./Amp. JD0 Period
12.460 V Y 0.630 V 2451957.20000 50.780000000000
The object was not found in astcheck.
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:31:53.73 -38:01:32.5: 12.42 +/- 0.04 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:31:53.73 -38:01:32.5: 12.48 +/- 0.05 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 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 03.4820* 09 31 53.73 -38 01 32.5 11.5 U Ant 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 J093154-3801.6,2461347.9820,11.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J093154-3801.6 20261103.4820 11.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 03.4820 2461347.9820 11.41 09:20:24.96 -31:58:32.7
259.18182 12.44132 galactic Pyx Second-epoch detections are separated by 0.2" and 7.4 pix
The object was found in VSX 1" ASAS J092025-3158.5
Type: MISC
# Max. Min./Amp. JD0 Period
11.710 V Y 0.910 V 2452744.40000 129.500000000000
The object was not found in astcheck.
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:20:24.96 -31:58:32.7: 12.38 +/- 0.03 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:20:24.96 -31:58:32.7: 12.41 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.40 +/- 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 J092025-3158.5,2461347.9820,11.41,0.05,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 J092025-3158.5 20261103.4820 11.41CV 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 03.4820 2461347.9820 12.11 09:10:02.78 -38:00:19.7
262.18321 6.77492 galactic Vel Second-epoch detections are separated by 2.2" and 7.5 pix
The object was found in VSX 2" ASAS J091003-3800.3
Type: MISC
# Max. Min./Amp. JD0 Period
9.270 Ic Y 0.993 Ic 2453339.90000 296.000000000000 M9
The object was not found in astcheck.
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:10:02.78 -38:00:19.7: 13.38 +/- 0.10 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:10:02.78 -38:00:19.7: 13.54 +/- 0.12 detection
Forced photometry reference-image weighted average: 13.45 +/- 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!
TCP 2026 11 03.4820* 09 10 02.78 -38 00 19.7 12.1 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 J091003-3800.3,2461347.9820,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J091003-3800.3 20261103.4820 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 03.4820 2461347.9820 12.29 09:38:49.66 -35:19:45.5
264.38842 12.75169 galactic Ant Second-epoch detections are separated by 0.2" and 7.3 pix
The object was found in VSX 1" ASASSN-V J093849.70-351944.6
Type: L
# Max. Min./Amp. JD0 Period
13.400 V 13.930 V
The object was not found in astcheck.
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:38:49.66 -35:19:45.5: 13.36 +/- 0.10 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:38:49.66 -35:19:45.5: 13.40 +/- 0.10 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!
TCP 2026 11 03.4820* 09 38 49.66 -35 19 45.5 12.3 U Ant 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J093849.70-351944.6,2461347.9820,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J093849.70-351944.6 20261103.4820 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 03.4820 2461347.9820 10.97 09:05:45.07 -37:39:38.5
261.35320 6.37714 galactic Vel Second-epoch detections are separated by 0.7" and 7.6 pix
The object was found in VSX 1" V0480 Vel
Type: SRB
# Max. Min./Amp. JD0 Period
12.700 V < 14.200 V 233.000000000000 M6
The object was not found in astcheck.
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:05:45.07 -37:39:38.5: 12.01 +/- 0.03 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:05:45.07 -37:39:38.5: 12.08 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.04 +/- 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!
TCP 2026 11 03.4820* 09 05 45.07 -37 39 38.5 11.0 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
V0480 Vel,2461347.9820,10.97,0.05,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
V0480 Vel 20261103.4820 10.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 03.4820 2461347.9820 12.29 09:00:07.66 -32:13:05.3
256.44601 9.08029 galactic Pyx Second-epoch detections are separated by 1.4" and 7.3 pix
The object was found in VSX 2" ASASSN-V J090007.60-321303.8
Type: SR
# Max. Min./Amp. JD0 Period
12.920 V 14.900 V 2457854.70000 257.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:00:07.66 -32:13:05.3: 13.36 +/- 0.09 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:00:07.66 -32:13:05.3: 13.26 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.31 +/- 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
ASASSN-V J090007.60-321303.8,2461347.9820,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J090007.60-321303.8 20261103.4820 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 03.4820 2461347.9820 11.99 09:58:21.75 -34:56:55.3
267.23606 15.66246 galactic Ant Second-epoch detections are separated by 0.4" and 7.1 pix
The object was found in VSX 4" ASASSN-V J095822.05-345654.9
Type: SR
# Max. Min./Amp. JD0 Period
12.810 V 14.490 V 2457131.00000 269.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:58:21.75 -34:56:55.3: 13.12 +/- 0.10 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:58:21.75 -34:56:55.3: 13.17 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.15 +/- 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!
TCP 2026 11 03.4820* 09 58 21.75 -34 56 55.3 12.0 U Ant 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J095822.05-345654.9,2461347.9820,11.99,0.05,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 J095822.05-345654.9 20261103.4820 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 03.4820 2461347.9820 12.24 09:13:48.30 -36:52:21.9
261.85550 8.09176 galactic Pyx Second-epoch detections are separated by 1.4" and 7.3 pix
The object was found in VSX 1" ASASSN-V J091348.19-365221.7
Type: L
# Max. Min./Amp. JD0 Period
12.990 V 13.650 V
The object was not found in astcheck.
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:13:48.30 -36:52:21.9: 13.15 +/- 0.08 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:13:48.30 -36:52:21.9: 13.21 +/- 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
ASASSN-V J091348.19-365221.7,2461347.9820,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J091348.19-365221.7 20261103.4820 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 03.4820 2461347.9820 12.21 09:28:31.43 -38:50:14.3
265.32910 8.79295 galactic Ant Second-epoch detections are separated by 1.4" and 7.6 pix
The object was found in VSX 1" ASASSN-V J092831.47-385015.1
Type: SR
# Max. Min./Amp. JD0 Period
14.530 g Y 0.690 g 2458626.51100 76.620000000000
The object was not found in astcheck.
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:28:31.43 -38:50:14.3: 13.11 +/- 0.09 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:28:31.43 -38:50:14.3: 13.41 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.23 +/- 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!
TCP 2026 11 03.4820* 09 28 31.43 -38 50 14.3 12.2 U Ant 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J092831.47-385015.1,2461347.9820,12.21,0.05,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
ASASSN-V J092831.47-385015.1 20261103.4820 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 03.4820 2461347.9820 10.27 09:42:54.37 -34:33:23.4
264.48475 13.88615 galactic Ant Second-epoch detections are separated by 0.6" and 7.2 pix
The object was found in VSX 1" ASAS J094255-3433.4
Type: MISC
# Max. Min./Amp. JD0 Period
11.730 V Y 0.410 V 2453185.50000 291.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:42:54.37 -34:33:23.4: 11.39 +/- 0.02 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:42:54.37 -34:33:23.4: 11.45 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.42 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin 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 03.4820* 09 42 54.37 -34 33 23.4 10.3 U Ant 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 J094255-3433.4,2461347.9820,10.27,0.05,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 J094255-3433.4 20261103.4820 10.27CV 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 03.4820 2461347.9820 12.15 09:14:59.87 -37:15:48.5
262.30774 7.99813 galactic Pyx Second-epoch detections are separated by 0.7" and 7.4 pix
The object was found in VSX 1" ASASSN-V J091459.84-371549.6
Type: L
# Max. Min./Amp. JD0 Period
13.370 V 13.960 V
The object was not found in astcheck.
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:14:59.87 -37:15:48.5: 13.05 +/- 0.08 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:14:59.87 -37:15:48.5: 13.17 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.11 +/- 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
ASASSN-V J091459.84-371549.6,2461347.9820,12.15,0.05,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 J091459.84-371549.6 20261103.4820 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 03.4820 2461347.9820 10.24 09:13:49.09 -38:07:08.0
262.77551 7.24233 galactic Vel Second-epoch detections are separated by 0.2" and 7.6 pix
The object was found in VSX 1" ASAS J091349-3807.2
Type: MISC
# Max. Min./Amp. JD0 Period
11.570 V Y 0.450 V 2452739.30000 489.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:13:49.09 -38:07:08.0: 11.17 +/- 0.01 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:13:49.09 -38:07:08.0: 11.26 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.22 +/- 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!
TCP 2026 11 03.4820* 09 13 49.09 -38 07 08.0 10.2 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 J091349-3807.2,2461347.9820,10.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J091349-3807.2 20261103.4820 10.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 03.4820 2461347.9820 9.99 09:23:39.86 -33:29:36.3
260.78525 11.88183 galactic Pyx Second-epoch detections are separated by 0.3" and 7.5 pix
The object was found in VSX 1" ASAS J092340-3329.6
Type: MISC
# Max. Min./Amp. JD0 Period
10.950 V Y 0.630 V 2452698.30000 1152.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:23:39.86 -33:29:36.3: 11.04 +/- 0.01 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:23:39.86 -33:29:36.3: 11.09 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.06 +/- 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
ASAS J092340-3329.6,2461347.9820,9.99,0.05,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 J092340-3329.6 20261103.4820 9.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 03.4820 2461347.9820 9.34 09:12:36.29 -36:37:13.3
261.50345 8.08754 galactic Pyx Second-epoch detections are separated by 0.6" and 7.4 pix
The object was found in VSX 1" ASAS J091236-3637.2
Type: MISC
# Max. Min./Amp. JD0 Period
10.210 V Y 0.890 V 2452093.60000 83.200000000000
The object was not found in astcheck.
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:12:36.29 -36:37:13.3: 10.43 +/- 0.01 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:12:36.29 -36:37:13.3: 10.50 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.47 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin 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 J091236-3637.2,2461347.9820,9.34,0.05,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 J091236-3637.2 20261103.4820 9.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 03.4820 2461347.9820 11.85 09:01:08.48 -36:30:30.1
259.87149 6.44739 galactic Pyx Second-epoch detections are separated by 0.6" and 7.6 pix
The object was found in VSX 1" ASASSN-V J090108.39-363029.3
Type: L
# Max. Min./Amp. JD0 Period
13.210 V 13.630 V
The object was not found in astcheck.
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:01:08.48 -36:30:30.1: 12.86 +/- 0.06 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:01:08.48 -36:30:30.1: 12.93 +/- 0.06 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 J090108.39-363029.3,2461347.9820,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J090108.39-363029.3 20261103.4820 11.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 03.4820 2461347.9820 12.22 09:29:56.61 -34:18:20.4
262.31376 12.23247 galactic Ant Second-epoch detections are separated by 0.8" and 7.5 pix
The object was found in VSX 1" ASASSN-V J092956.70-341820.0
Type: SR
# Max. Min./Amp. JD0 Period
13.390 V 14.150 V 2457911.60000 64.600000000000
The object was not found in astcheck.
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:29:56.61 -34:18:20.4: 13.71 +/- 0.12 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:29:56.61 -34:18:20.4: 13.61 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.66 +/- 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!
TCP 2026 11 03.4820* 09 29 56.61 -34 18 20.4 12.2 U Ant 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J092956.70-341820.0,2461347.9820,12.22,0.05,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 J092956.70-341820.0 20261103.4820 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461139.64358051 09.04.2026 03:26:35.356 /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits
First image: 2461139.64358051 09.04.2026 03:26:35.356 /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits
Last image: 2461347.98225797 03.11.2026 11:34:17.089 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pyx-02-Q1b1x1_053531_TTUQ1b1x1_1550823_YDJ5pKlT/fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 57
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.13
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): 10287
Objects passed selection criteria: 10280
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 9658.75
Average stars matched: 9241.75 (95.6827 %)
Memory usage VmPeak: 235680 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 05:40:42 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: 2461139.64358051 09.04.2026 03:26:35.356 /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits
First image: 2461139.64358051 09.04.2026 03:26:35.356 /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits
Last image: 2461347.98225797 03.11.2026 11:34:17.089 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pyx-02-Q1b1x1_053531_TTUQ1b1x1_1550823_YDJ5pKlT/fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 161
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.79
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: 38 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): 78667
Objects passed selection criteria: 78501
Measurements per detected object (mean, median, min, max): 3.3 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.3 4.0 2 4
Average stars detected per image: 68768.2
Average stars matched: 66092.8 (96.1094 %)
Memory usage VmPeak: 569424 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 05:42:54 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/Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pyx-02-Q1b1x1_053531_TTUQ1b1x1_1550823_YDJ5pKlT/fd_Pyx-02-Q1b1x1_2026-11-03_05-33-28_20.00sec_-0.00C_LIGHTs_0557.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pyx-02-Q1b1x1_053531_TTUQ1b1x1_1550823_YDJ5pKlT/fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558.fits
SExtractor catalog cache: saved Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits.cat to cache
SExtractor catalog cache: saved Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.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/Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pyx-02-Q1b1x1_053531_TTUQ1b1x1_1550823_YDJ5pKlT/fd_Pyx-02-Q1b1x1_2026-11-03_05-33-28_20.00sec_-0.00C_LIGHTs_0557.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pyx-02-Q1b1x1_053531_TTUQ1b1x1_1550823_YDJ5pKlT/fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558.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: 2461347.98169601
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_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits exists and is non-empty
wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits exists and is non-empty
wcs_fd_Pyx-02-Q1b1x1_2026-11-03_05-33-28_20.00sec_-0.00C_LIGHTs_0557.fits exists and is non-empty
wcs_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits (1st reference image)
verification OK: wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits
Image size: 937.5'x625.2' 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: 09:23:38.619 -34:01:02.00 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_Pyx-02-Q1b1x1_2026-11-03_05-33-28_20.00sec_-0.00C_LIGHTs_0557.fits (1st new image)
verification OK: wcs_fd_Pyx-02-Q1b1x1_2026-11-03_05-33-28_20.00sec_-0.00C_LIGHTs_0557.fits
Image size: 941.6'x627.6' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 09:23:22.962 -34:00:17.54 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 09:23:38.619 -34:01:02.00
Second-epoch image center 09:23:22.962 -34:00:17.54
Angular distance between the image centers 0.0555 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558.fits (2nd new image)
verification OK: wcs_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558.fits
Image size: 941.5'x627.5' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 09:23:22.370 -33:59:33.71 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 09:23:38.619 -34:01:02.00
Second-epoch image center 09:23:22.370 -33:59:33.71
Angular distance between the image centers 0.0612 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 09:23:22.962 -34:00:17.54
Second-epoch second image center 09:23:22.370 -33:59:33.71
Angular distance between the image centers 0.01235 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/Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits &> /tmp/tmp.YqnriAH2uA
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits &> /tmp/tmp.drkzDvflZd
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pyx-02-Q1b1x1_053531_TTUQ1b1x1_1550823_YDJ5pKlT/fd_Pyx-02-Q1b1x1_2026-11-03_05-33-28_20.00sec_-0.00C_LIGHTs_0557.fits &> /tmp/tmp.1NUw4qVq52
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pyx-02-Q1b1x1_053531_TTUQ1b1x1_1550823_YDJ5pKlT/fd_Pyx-02-Q1b1x1_2026-11-03_05-33-28_20.00sec_-0.00C_LIGHTs_0557.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pyx-02-Q1b1x1_053531_TTUQ1b1x1_1550823_YDJ5pKlT/fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558.fits &> /tmp/tmp.qEMmo9zgTy
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pyx-02-Q1b1x1_053531_TTUQ1b1x1_1550823_YDJ5pKlT/fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558.fits
Calibrating the magnitude scale
Found non-empty wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.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_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits and wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.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_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits and wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits.wcscat
Found non-empty wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits and wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits.wcscat
The reference image (wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits) and catalog (wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits.wcscat) found
'wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits.wcscat' -> 'wcsmag.cat'
Read 9578 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 131.0027 to 150.9550 deg, Dec -39.2955 to -28.3714 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 131.0027 to 150.9550 deg, Dec -39.2955 to -28.3714 deg
Loaded 17623 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): 7863 out of 8091 total matches.
Matched with Tycho-2 8091 out of 9578 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.446800
a=0.000000 b=1.000000 c=22.446800
From vast_summary.log: estimated ref. image limiting mag.: -8.13
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.32
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.32
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 9578 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 131.0027 to 150.9550 deg, Dec -39.2955 to -28.3714 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 131.0027 to 150.9550 deg, Dec -39.2955 to -28.3714 deg
Loaded 17623 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): 7863 out of 8091 total matches.
Matched with Tycho-2 8091 out of 9578 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits
Forced-photometry filter: calibrated wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits -> calib.txt_param_ref_wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits (aperture=6.3)
Read 9580 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 130.9665 to 150.9161 deg, Dec -39.2972 to -28.3758 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 130.9665 to 150.9161 deg, Dec -39.2972 to -28.3758 deg
Loaded 17626 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): 4986 out of 5146 total matches.
Matched with Tycho-2 5146 out of 9580 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits
Forced-photometry filter: calibrated wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits -> calib.txt_param_ref_wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits (aperture=6.3)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 56 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.4 pix Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits
2.4 pix Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits
4.0 pix fd_Pyx-02-Q1b1x1_2026-11-03_05-33-28_20.00sec_-0.00C_LIGHTs_0557.fits
4.0 pix fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558.fits
Limiting magnitude estimates:
14.3 mag. Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits
14.3 mag. Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits
14.0 mag. fd_Pyx-02-Q1b1x1_2026-11-03_05-33-28_20.00sec_-0.00C_LIGHTs_0557.fits
14.0 mag. fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 11.2 (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.YqnriAH2uA (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/Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.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_Pyx-02-Q1b1x1_053531_TTUQ1b1x1_1550823_YDJ5pKlT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits' -> 'wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.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/Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits
WCS_IMAGE_NAME=wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits
WCS-calibrated image found: wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits
Checking if the catalog wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits.wcscat corresponding to the image wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits alredy exist and is non-empty...
Catalog wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits.wcscat corresponding to the image wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits
WCS catalog name: wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.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=682, bad_region=0, passed=9578
Got 9578 stars (including 8882 good ones) from the SExtractor catalog wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits.wcscat
util/solve_plate_with_UCAC5 got 9578 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 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: 4886 matched stars entering correct_measured_positions(), 4886 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4886 matched stars entering correct_measured_positions(), 9578 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
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 4922 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4888 matched stars entering correct_measured_positions(), 9578 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Accuracy estimation diagnostic: 4888 matched stars entering correct_measured_positions(), 9578 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Excluding outliers - 4888 stars left (next iteration limit 5374)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits N_match=4888 sigma_overall_arcsec=0.568 sigma_q1_arcsec=0.426 sigma_q2_arcsec=0.674 sigma_q3_arcsec=0.489 sigma_q4_arcsec=0.708 n_q1=1031 n_q2=1301 n_q3=1130 n_q4=1426 worst_quadrant_to_overall_ratio=1.245
WCS_HEADER_DIAG: file=Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits selection=current_pairs N_selected=4888 N_valid=4888 bias_ra_arcsec=0.004 bias_dec_arcsec=0.010 median_sep_arcsec=0.471 p95_sep_arcsec=2.527 n_q1=1031 n_q2=1301 n_q3=1130 n_q4=1426 occupied_cells_4x4=16/16
The image catalog is written to wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits -region wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.drkzDvflZd (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/Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.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_Pyx-02-Q1b1x1_053531_TTUQ1b1x1_1550823_YDJ5pKlT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits' -> 'wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.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/Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits
WCS_IMAGE_NAME=wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits
WCS-calibrated image found: wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits
Checking if the catalog wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits.wcscat corresponding to the image wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits alredy exist and is non-empty...
Catalog wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits.wcscat corresponding to the image wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits
WCS catalog name: wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.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=679, bad_region=0, passed=9580
Got 9580 stars (including 8893 good ones) from the SExtractor catalog wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits.wcscat
util/solve_plate_with_UCAC5 got 9580 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 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: 4884 matched stars entering correct_measured_positions(), 4884 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4884 matched stars entering correct_measured_positions(), 9580 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
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 4922 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4887 matched stars entering correct_measured_positions(), 9580 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Accuracy estimation diagnostic: 4887 matched stars entering correct_measured_positions(), 9580 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Excluding outliers - 4887 stars left (next iteration limit 5372)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits N_match=4887 sigma_overall_arcsec=0.600 sigma_q1_arcsec=0.495 sigma_q2_arcsec=0.692 sigma_q3_arcsec=0.533 sigma_q4_arcsec=0.719 n_q1=1032 n_q2=1293 n_q3=1129 n_q4=1433 worst_quadrant_to_overall_ratio=1.198
WCS_HEADER_DIAG: file=Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits selection=current_pairs N_selected=4887 N_valid=4887 bias_ra_arcsec=0.020 bias_dec_arcsec=0.611 median_sep_arcsec=4.277 p95_sep_arcsec=10.327 n_q1=1032 n_q2=1293 n_q3=1129 n_q4=1433 occupied_cells_4x4=16/16
The image catalog is written to wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits -region wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.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.1NUw4qVq52 (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_Pyx-02-Q1b1x1_053531_TTUQ1b1x1_1550823_YDJ5pKlT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pyx-02-Q1b1x1_053531_TTUQ1b1x1_1550823_YDJ5pKlT/fd_Pyx-02-Q1b1x1_2026-11-03_05-33-28_20.00sec_-0.00C_LIGHTs_0557.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pyx-02-Q1b1x1_053531_TTUQ1b1x1_1550823_YDJ5pKlT/fd_Pyx-02-Q1b1x1_2026-11-03_05-33-28_20.00sec_-0.00C_LIGHTs_0557.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pyx-02-Q1b1x1_053531_TTUQ1b1x1_1550823_YDJ5pKlT/fd_Pyx-02-Q1b1x1_2026-11-03_05-33-28_20.00sec_-0.00C_LIGHTs_0557.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pyx-02-Q1b1x1_053531_TTUQ1b1x1_1550823_YDJ5pKlT/fd_Pyx-02-Q1b1x1_2026-11-03_05-33-28_20.00sec_-0.00C_LIGHTs_0557.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pyx-02-Q1b1x1_053531_TTUQ1b1x1_1550823_YDJ5pKlT/fd_Pyx-02-Q1b1x1_2026-11-03_05-33-28_20.00sec_-0.00C_LIGHTs_0557.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_Pyx-02-Q1b1x1_053531_TTUQ1b1x1_1550823_YDJ5pKlT/fd_Pyx-02-Q1b1x1_2026-11-03_05-33-28_20.00sec_-0.00C_LIGHTs_0557.fits
WCS_IMAGE_NAME=wcs_fd_Pyx-02-Q1b1x1_2026-11-03_05-33-28_20.00sec_-0.00C_LIGHTs_0557.fits
WCS-calibrated image found: wcs_fd_Pyx-02-Q1b1x1_2026-11-03_05-33-28_20.00sec_-0.00C_LIGHTs_0557.fits
Checking if the catalog wcs_fd_Pyx-02-Q1b1x1_2026-11-03_05-33-28_20.00sec_-0.00C_LIGHTs_0557.fits.wcscat corresponding to the image wcs_fd_Pyx-02-Q1b1x1_2026-11-03_05-33-28_20.00sec_-0.00C_LIGHTs_0557.fits alredy exist and is non-empty...
Catalog wcs_fd_Pyx-02-Q1b1x1_2026-11-03_05-33-28_20.00sec_-0.00C_LIGHTs_0557.fits.wcscat corresponding to the image wcs_fd_Pyx-02-Q1b1x1_2026-11-03_05-33-28_20.00sec_-0.00C_LIGHTs_0557.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Pyx-02-Q1b1x1_2026-11-03_05-33-28_20.00sec_-0.00C_LIGHTs_0557.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_Pyx-02-Q1b1x1_053531_TTUQ1b1x1_1550823_YDJ5pKlT/fd_Pyx-02-Q1b1x1_2026-11-03_05-33-28_20.00sec_-0.00C_LIGHTs_0557.fits
WCS catalog name: wcs_fd_Pyx-02-Q1b1x1_2026-11-03_05-33-28_20.00sec_-0.00C_LIGHTs_0557.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=418, bad_region=0, passed=9843
Got 9843 stars (including 9420 good ones) from the SExtractor catalog wcs_fd_Pyx-02-Q1b1x1_2026-11-03_05-33-28_20.00sec_-0.00C_LIGHTs_0557.fits.wcscat
util/solve_plate_with_UCAC5 got 9843 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (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 -39.4 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: 4873 matched stars entering correct_measured_positions(), 4875 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4873 matched stars entering correct_measured_positions(), 9843 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
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 -39.4 to -28.2)
Done reading UCAC5 zone files...
Matched 4919 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4878 matched stars entering correct_measured_positions(), 9843 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Accuracy estimation diagnostic: 4878 matched stars entering correct_measured_positions(), 9843 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 4878 stars left (next iteration limit 5360)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4878 robust_rms=12.369 arcsec worst_region_rms=26.739 arcsec outer_annulus_rms=26.739 arcsec
SIP_REFIT: SIP order 3 trial: matched=4878 robust_rms=0.667 arcsec worst_region_rms=1.030 arcsec outer_annulus_rms=1.030 arcsec
SIP_REFIT: SIP order 5 trial: matched=4878 robust_rms=0.507 arcsec worst_region_rms=0.807 arcsec outer_annulus_rms=0.807 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4878 robust_rms_before=1.353 arcsec robust_rms_before_corrected=0.511 arcsec robust_rms_after=0.507 arcsec worst_region_rms_before=0.868 worst_region_rms_after=0.807 outer_annulus_rms_before=1.824 outer_annulus_rms_after=0.807
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.868 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Pyx-02-Q1b1x1_2026-11-03_05-33-28_20.00sec_-0.00C_LIGHTs_0557.fits worst_region_rms_kept=0.868 arcsec robust_rms_kept=0.511 arcsec matched=4878
WCS_QUALITY_DIAG: file=fd_Pyx-02-Q1b1x1_2026-11-03_05-33-28_20.00sec_-0.00C_LIGHTs_0557.fits N_match=4878 sigma_overall_arcsec=0.488 sigma_q1_arcsec=0.629 sigma_q2_arcsec=0.581 sigma_q3_arcsec=0.385 sigma_q4_arcsec=0.373 n_q1=1430 n_q2=1031 n_q3=1390 n_q4=1027 worst_quadrant_to_overall_ratio=1.289
WCS_HEADER_DIAG: file=fd_Pyx-02-Q1b1x1_2026-11-03_05-33-28_20.00sec_-0.00C_LIGHTs_0557.fits selection=current_pairs N_selected=4878 N_valid=4878 bias_ra_arcsec=0.995 bias_dec_arcsec=-0.368 median_sep_arcsec=1.231 p95_sep_arcsec=3.381 n_q1=1430 n_q2=1031 n_q3=1390 n_q4=1027 occupied_cells_4x4=16/16
The image catalog is written to wcs_fd_Pyx-02-Q1b1x1_2026-11-03_05-33-28_20.00sec_-0.00C_LIGHTs_0557.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Pyx-02-Q1b1x1_2026-11-03_05-33-28_20.00sec_-0.00C_LIGHTs_0557.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pyx-02-Q1b1x1_053531_TTUQ1b1x1_1550823_YDJ5pKlT/fd_Pyx-02-Q1b1x1_2026-11-03_05-33-28_20.00sec_-0.00C_LIGHTs_0557.fits -region wcs_fd_Pyx-02-Q1b1x1_2026-11-03_05-33-28_20.00sec_-0.00C_LIGHTs_0557.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Pyx-02-Q1b1x1_2026-11-03_05-33-28_20.00sec_-0.00C_LIGHTs_0557.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.qEMmo9zgTy (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_Pyx-02-Q1b1x1_053531_TTUQ1b1x1_1550823_YDJ5pKlT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pyx-02-Q1b1x1_053531_TTUQ1b1x1_1550823_YDJ5pKlT/fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pyx-02-Q1b1x1_053531_TTUQ1b1x1_1550823_YDJ5pKlT/fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pyx-02-Q1b1x1_053531_TTUQ1b1x1_1550823_YDJ5pKlT/fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pyx-02-Q1b1x1_053531_TTUQ1b1x1_1550823_YDJ5pKlT/fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pyx-02-Q1b1x1_053531_TTUQ1b1x1_1550823_YDJ5pKlT/fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558.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_Pyx-02-Q1b1x1_053531_TTUQ1b1x1_1550823_YDJ5pKlT/fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558.fits
WCS_IMAGE_NAME=wcs_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558.fits
WCS-calibrated image found: wcs_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558.fits
Checking if the catalog wcs_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558.fits.wcscat corresponding to the image wcs_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558.fits alredy exist and is non-empty...
Catalog wcs_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558.fits.wcscat corresponding to the image wcs_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558.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_Pyx-02-Q1b1x1_053531_TTUQ1b1x1_1550823_YDJ5pKlT/fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558.fits
WCS catalog name: wcs_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558.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=424, bad_region=0, passed=9868
Got 9868 stars (including 9437 good ones) from the SExtractor catalog wcs_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558.fits.wcscat
util/solve_plate_with_UCAC5 got 9868 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 310 (Dec -39.3 to -28.2)
Done reading UCAC5 zone files...
Matched 4913 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4874 matched stars entering correct_measured_positions(), 4875 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4874 matched stars entering correct_measured_positions(), 9868 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 310 (Dec -39.3 to -28.2)
Done reading UCAC5 zone files...
Matched 4917 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4878 matched stars entering correct_measured_positions(), 9868 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Accuracy estimation diagnostic: 4878 matched stars entering correct_measured_positions(), 9868 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Excluding outliers - 4878 stars left (next iteration limit 5361)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4878 robust_rms=12.405 arcsec worst_region_rms=26.766 arcsec outer_annulus_rms=26.766 arcsec
SIP_REFIT: SIP order 3 trial: matched=4878 robust_rms=0.600 arcsec worst_region_rms=0.973 arcsec outer_annulus_rms=0.973 arcsec
SIP_REFIT: SIP order 5 trial: matched=4878 robust_rms=0.495 arcsec worst_region_rms=0.789 arcsec outer_annulus_rms=0.789 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4878 robust_rms_before=1.376 arcsec robust_rms_before_corrected=0.505 arcsec robust_rms_after=0.495 arcsec worst_region_rms_before=0.859 worst_region_rms_after=0.789 outer_annulus_rms_before=1.839 outer_annulus_rms_after=0.789
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.859 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558.fits worst_region_rms_kept=0.859 arcsec robust_rms_kept=0.505 arcsec matched=4878
WCS_QUALITY_DIAG: file=fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558.fits N_match=4878 sigma_overall_arcsec=0.476 sigma_q1_arcsec=0.599 sigma_q2_arcsec=0.570 sigma_q3_arcsec=0.400 sigma_q4_arcsec=0.359 n_q1=1435 n_q2=1028 n_q3=1386 n_q4=1029 worst_quadrant_to_overall_ratio=1.259
WCS_HEADER_DIAG: file=fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558.fits selection=current_pairs N_selected=4878 N_valid=4878 bias_ra_arcsec=1.063 bias_dec_arcsec=-0.324 median_sep_arcsec=1.250 p95_sep_arcsec=3.533 n_q1=1435 n_q2=1028 n_q3=1386 n_q4=1029 occupied_cells_4x4=16/16
The image catalog is written to wcs_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pyx-02-Q1b1x1_053531_TTUQ1b1x1_1550823_YDJ5pKlT/fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558.fits -region wcs_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558.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_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits to local_wcs_cache/
'wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits' -> 'local_wcs_cache/wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits'
Saving the final (post-refit) wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits to local_wcs_cache/
'wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits' -> 'local_wcs_cache/wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits'
Saving the final (post-refit) wcs_fd_Pyx-02-Q1b1x1_2026-11-03_05-33-28_20.00sec_-0.00C_LIGHTs_0557.fits to local_wcs_cache/
'wcs_fd_Pyx-02-Q1b1x1_2026-11-03_05-33-28_20.00sec_-0.00C_LIGHTs_0557.fits' -> 'local_wcs_cache/wcs_fd_Pyx-02-Q1b1x1_2026-11-03_05-33-28_20.00sec_-0.00C_LIGHTs_0557.fits'
Saving the final (post-refit) wcs_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558.fits to local_wcs_cache/
'wcs_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558.fits' -> 'local_wcs_cache/wcs_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits sigma_overall=0.568 worst_q_ratio=1.245
ref2=Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits sigma_overall=0.600 worst_q_ratio=1.198
new1=fd_Pyx-02-Q1b1x1_2026-11-03_05-33-28_20.00sec_-0.00C_LIGHTs_0557.fits sigma_overall=0.488 worst_q_ratio=1.289
new2=fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558.fits sigma_overall=0.476 worst_q_ratio=1.259
reference average sigma_overall=0.584 worst_q_ratio=1.2215
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094_astrometric_residuals.png (4888 matched stars from wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.51 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095_astrometric_residuals.png (4887 matched stars from wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.53 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Pyx-02-Q1b1x1_2026-11-03_05-33-28_20.00sec_-0.00C_LIGHTs_0557_astrometric_residuals.png (4878 matched stars from wcs_fd_Pyx-02-Q1b1x1_2026-11-03_05-33-28_20.00sec_-0.00C_LIGHTs_0557.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.46 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558_astrometric_residuals.png (4878 matched stars from wcs_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.45 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Pyx-02-Q1b1x1_2026-11-03_05-33-28_20.00sec_-0.00C_LIGHTs_0557.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Pyx-02-Q1b1x1_2026-11-03_05-33-28_20.00sec_-0.00C_LIGHTs_0557.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pyx-02-Q1b1x1_053531_TTUQ1b1x1_1550823_YDJ5pKlT/wcs_fd_Pyx-02-Q1b1x1_2026-11-03_05-33-28_20.00sec_-0.00C_LIGHTs_0557.fits'
Saving fully-calibrated image wcs_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pyx-02-Q1b1x1_053531_TTUQ1b1x1_1550823_YDJ5pKlT/wcs_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558.fits'
Preparing the HTML report for the field Pyx-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:18:47.01 -35:44:18.1: 11.60 +/- 0.02 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:10:14.73 -37:55:22.6: 11.60 +/- 0.02 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 08:51:18.09 -36:22:08.8: 11.79 +/- 0.03 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:36:19.65 -37:38:56.3: 11.63 +/- 0.03 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:57:01.14 -35:57:42.2: 13.08 +/- 0.12 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:11:18.82 -31:42:21.9: 11.49 +/- 0.02 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:09:00.84 -32:17:47.2: 11.19 +/- 0.01 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:05:45.09 -37:39:39.0: 11.94 +/- 0.03 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:19:09.07 -32:55:28.4: 11.12 +/- 0.01 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:15:27.14 -32:38:06.0: 11.35 +/- 0.01 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 08:51:18.09 -36:22:08.8: 11.75 +/- 0.03 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:36:19.65 -37:38:56.3: 11.73 +/- 0.03 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:57:01.14 -35:57:42.2: 13.04 +/- 0.11 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:18:47.01 -35:44:18.1: 11.61 +/- 0.02 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:10:14.73 -37:55:22.6: 11.59 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.77 +/- 0.02
Forced photometry reference-image weighted average: 13.06 +/- 0.08
Forced photometry filter KEPT candidate at 09:57:01.14 -35:57:42.2: ref_mag=13.06 +/- 0.08 new_mean_mag=10.6975 delta=2.37 (need > 0.90)
Forced photometry reference-image weighted average: 11.68 +/- 0.02
Forced photometry filter REJECTED candidate at 08:51:18.09 -36:22:08.8: ref_mag=11.77 +/- 0.02 new_mean_mag=11.0373 delta=0.73 (need > 0.90)
Forced photometry reference-image weighted average: 11.60 +/- 0.01
Forced photometry filter REJECTED candidate at 09:36:19.65 -37:38:56.3: ref_mag=11.68 +/- 0.02 new_mean_mag=11.0845 delta=0.59 (need > 0.90)
Forced photometry filter KEPT candidate at 09:18:47.01 -35:44:18.1: ref_mag=11.60 +/- 0.01 new_mean_mag=10.5672 delta=1.04 (need > 0.90)
Forced photometry reference-image weighted average: 11.59 +/- 0.02
Forced photometry filter REJECTED candidate at 09:10:14.73 -37:55:22.6: ref_mag=11.59 +/- 0.02 new_mean_mag=11.0756 delta=0.52 (need > 0.90)
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:11:18.82 -31:42:21.9: 11.52 +/- 0.02 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:09:00.84 -32:17:47.2: 11.16 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.51 +/- 0.01
Forced photometry filter REJECTED candidate at 09:11:18.82 -31:42:21.9: ref_mag=11.51 +/- 0.01 new_mean_mag=11.0438 delta=0.46 (need > 0.90)
Forced photometry reference-image weighted average: 11.17 +/- 0.01
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:05:45.09 -37:39:39.0: 11.94 +/- 0.03 detection
Forced photometry filter REJECTED candidate at 09:09:00.84 -32:17:47.2: ref_mag=11.17 +/- 0.01 new_mean_mag=11.0926 delta=0.08 (need > 0.90)
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:19:09.07 -32:55:28.4: 11.15 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.94 +/- 0.02
Forced photometry filter REJECTED candidate at 09:05:45.09 -37:39:39.0: ref_mag=11.94 +/- 0.02 new_mean_mag=11.0799 delta=0.86 (need > 0.90)
Forced photometry reference-image weighted average: 11.13 +/- 0.01
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:15:27.14 -32:38:06.0: 11.33 +/- 0.01 detection
Forced photometry filter REJECTED candidate at 09:19:09.07 -32:55:28.4: ref_mag=11.13 +/- 0.01 new_mean_mag=11.0944 delta=0.04 (need > 0.90)
Forced photometry reference-image weighted average: 11.34 +/- 0.01
Forced photometry filter REJECTED candidate at 09:15:27.14 -32:38:06.0: ref_mag=11.34 +/- 0.01 new_mean_mag=11.0897 delta=0.25 (need > 0.90)
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:32:06.79 -33:27:14.8: 11.20 +/- 0.01 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:44:21.65 -29:20:25.0: 11.30 +/- 0.02 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:13:33.31 -33:36:59.4: 11.19 +/- 0.01 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:08:41.15 -34:28:17.3: 11.18 +/- 0.01 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:19:10.21 -33:00:05.7: 11.13 +/- 0.01 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:33:24.69 -36:42:56.5: 11.39 +/- 0.02 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:15:20.50 -33:37:38.3: 11.26 +/- 0.01 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:21:57.24 -32:55:15.8: 11.23 +/- 0.01 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:32:06.79 -33:27:14.8: 11.21 +/- 0.01 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:44:21.65 -29:20:25.0: 11.29 +/- 0.02 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:13:33.31 -33:36:59.4: 11.18 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.20 +/- 0.01
Forced photometry filter REJECTED candidate at 09:32:06.79 -33:27:14.8: ref_mag=11.20 +/- 0.01 new_mean_mag=11.1372 delta=0.07 (need > 0.90)
Forced photometry reference-image weighted average: 11.30 +/- 0.01
Forced photometry reference-image weighted average: 11.19 +/- 0.01
Forced photometry filter REJECTED candidate at 09:44:21.65 -29:20:25.0: ref_mag=11.30 +/- 0.01 new_mean_mag=11.1647 delta=0.13 (need > 0.90)
Forced photometry filter REJECTED candidate at 09:13:33.31 -33:36:59.4: ref_mag=11.19 +/- 0.01 new_mean_mag=11.1652 delta=0.02 (need > 0.90)
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:08:41.15 -34:28:17.3: 11.22 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.20 +/- 0.01
Forced photometry filter REJECTED candidate at 09:08:41.15 -34:28:17.3: ref_mag=11.20 +/- 0.01 new_mean_mag=11.1717 delta=0.03 (need > 0.90)
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:33:24.69 -36:42:56.5: 11.44 +/- 0.02 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:19:10.21 -33:00:05.7: 11.13 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.41 +/- 0.01
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:15:20.50 -33:37:38.3: 11.32 +/- 0.01 detection
Forced photometry filter REJECTED candidate at 09:33:24.69 -36:42:56.5: ref_mag=11.41 +/- 0.01 new_mean_mag=11.1633 delta=0.25 (need > 0.90)
Forced photometry reference-image weighted average: 11.13 +/- 0.01
Forced photometry reference-image weighted average: 11.29 +/- 0.01
Forced photometry filter REJECTED candidate at 09:19:10.21 -33:00:05.7: ref_mag=11.13 +/- 0.01 new_mean_mag=11.1424 delta=-0.01 (need > 0.90)
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:21:57.24 -32:55:15.8: 11.32 +/- 0.01 detection
Forced photometry filter REJECTED candidate at 09:15:20.50 -33:37:38.3: ref_mag=11.29 +/- 0.01 new_mean_mag=11.1642 delta=0.13 (need > 0.90)
Forced photometry reference-image weighted average: 11.27 +/- 0.01
Forced photometry filter REJECTED candidate at 09:21:57.24 -32:55:15.8: ref_mag=11.27 +/- 0.01 new_mean_mag=11.1795 delta=0.09 (need > 0.90)
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:31:04.51 -34:29:53.0: 11.58 +/- 0.02 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:37:49.89 -37:36:13.1: 11.54 +/- 0.02 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:21:37.83 -34:45:09.4: 11.26 +/- 0.01 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:19:58.86 -33:17:22.2: 11.17 +/- 0.01 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:04:32.41 -32:22:51.3: 11.75 +/- 0.02 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:16:13.01 -34:18:43.0: 11.21 +/- 0.01 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:20:13.62 -33:46:10.5: 11.23 +/- 0.01 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:21:45.38 -32:51:38.8: 11.28 +/- 0.01 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:31:04.51 -34:29:53.0: 11.59 +/- 0.02 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:21:45.38 -32:51:38.8: 11.35 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.59 +/- 0.01
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:19:58.86 -33:17:22.2: 11.22 +/- 0.01 detection
Forced photometry filter REJECTED candidate at 09:31:04.51 -34:29:53.0: ref_mag=11.59 +/- 0.01 new_mean_mag=11.2544 delta=0.33 (need > 0.90)
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:37:49.89 -37:36:13.1: 11.56 +/- 0.02 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:21:37.83 -34:45:09.4: 11.29 +/- 0.01 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:04:32.41 -32:22:51.3: 11.76 +/- 0.02 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:16:13.01 -34:18:43.0: 11.23 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.31 +/- 0.01
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:20:13.62 -33:46:10.5: 11.27 +/- 0.01 detection
Forced photometry filter REJECTED candidate at 09:21:45.38 -32:51:38.8: ref_mag=11.31 +/- 0.01 new_mean_mag=11.2612 delta=0.05 (need > 0.90)
Forced photometry reference-image weighted average: 11.19 +/- 0.01
Forced photometry reference-image weighted average: 11.55 +/- 0.02
Forced photometry reference-image weighted average: 11.28 +/- 0.01
Forced photometry filter REJECTED candidate at 09:19:58.86 -33:17:22.2: ref_mag=11.19 +/- 0.01 new_mean_mag=11.2367 delta=-0.04 (need > 0.90)
Forced photometry reference-image weighted average: 11.75 +/- 0.02
Forced photometry filter REJECTED candidate at 09:37:49.89 -37:36:13.1: ref_mag=11.55 +/- 0.02 new_mean_mag=11.2254 delta=0.32 (need > 0.90)
Forced photometry filter REJECTED candidate at 09:21:37.83 -34:45:09.4: ref_mag=11.28 +/- 0.01 new_mean_mag=11.2063 delta=0.07 (need > 0.90)
Forced photometry reference-image weighted average: 11.25 +/- 0.01
Forced photometry reference-image weighted average: 11.22 +/- 0.01
Forced photometry filter REJECTED candidate at 09:04:32.41 -32:22:51.3: ref_mag=11.75 +/- 0.02 new_mean_mag=11.2577 delta=0.50 (need > 0.90)
Forced photometry filter REJECTED candidate at 09:16:13.01 -34:18:43.0: ref_mag=11.22 +/- 0.01 new_mean_mag=11.2327 delta=-0.01 (need > 0.90)
Forced photometry filter REJECTED candidate at 09:20:13.62 -33:46:10.5: ref_mag=11.25 +/- 0.01 new_mean_mag=11.2415 delta=0.01 (need > 0.90)
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:18:00.36 -32:03:32.2: 11.23 +/- 0.01 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:12:40.27 -34:53:34.7: 11.31 +/- 0.02 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:19:20.28 -32:10:46.0: 11.28 +/- 0.01 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:17:26.09 -32:11:40.7: 11.33 +/- 0.01 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:24:20.52 -30:18:02.4: 11.42 +/- 0.02 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:14:55.64 -33:38:08.8: 11.22 +/- 0.01 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:09:38.06 -33:11:32.6: 11.33 +/- 0.01 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:19:03.76 -33:16:48.1: 11.27 +/- 0.01 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:19:20.28 -32:10:46.0: 11.30 +/- 0.01 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:18:00.36 -32:03:32.2: 11.28 +/- 0.01 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:12:40.27 -34:53:34.7: 11.38 +/- 0.02 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:14:55.64 -33:38:08.8: 11.30 +/- 0.02 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:17:26.09 -32:11:40.7: 11.37 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.29 +/- 0.01
Forced photometry reference-image weighted average: 11.26 +/- 0.01
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:09:38.06 -33:11:32.6: 11.32 +/- 0.01 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:24:20.52 -30:18:02.4: 11.40 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.35 +/- 0.01
Forced photometry filter REJECTED candidate at 09:19:20.28 -32:10:46.0: ref_mag=11.29 +/- 0.01 new_mean_mag=11.2693 delta=0.02 (need > 0.90)
Forced photometry filter REJECTED candidate at 09:18:00.36 -32:03:32.2: ref_mag=11.26 +/- 0.01 new_mean_mag=11.2454 delta=0.01 (need > 0.90)
Forced photometry filter REJECTED candidate at 09:12:40.27 -34:53:34.7: ref_mag=11.35 +/- 0.01 new_mean_mag=11.2579 delta=0.09 (need > 0.90)
Forced photometry reference-image weighted average: 11.35 +/- 0.01
Forced photometry reference-image weighted average: 11.25 +/- 0.01
Forced photometry reference-image weighted average: 11.41 +/- 0.01
Forced photometry reference-image weighted average: 11.33 +/- 0.01
Forced photometry filter REJECTED candidate at 09:17:26.09 -32:11:40.7: ref_mag=11.35 +/- 0.01 new_mean_mag=11.2992 delta=0.05 (need > 0.90)
Forced photometry filter REJECTED candidate at 09:14:55.64 -33:38:08.8: ref_mag=11.25 +/- 0.01 new_mean_mag=11.2467 delta=0.01 (need > 0.90)
Forced photometry filter REJECTED candidate at 09:24:20.52 -30:18:02.4: ref_mag=11.41 +/- 0.01 new_mean_mag=11.2433 delta=0.16 (need > 0.90)
Forced photometry filter REJECTED candidate at 09:09:38.06 -33:11:32.6: ref_mag=11.33 +/- 0.01 new_mean_mag=11.2399 delta=0.09 (need > 0.90)
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:19:03.76 -33:16:48.1: 11.34 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.31 +/- 0.01
Forced photometry filter REJECTED candidate at 09:19:03.76 -33:16:48.1: ref_mag=11.31 +/- 0.01 new_mean_mag=11.2764 delta=0.03 (need > 0.90)
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:17:21.02 -30:37:07.1: 11.34 +/- 0.02 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:26:36.10 -34:28:07.3: 11.24 +/- 0.01 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:20:38.78 -32:39:53.3: 11.25 +/- 0.01 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 08:53:22.86 -35:54:14.1: 11.50 +/- 0.02 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:10:04.11 -33:02:07.6: 11.44 +/- 0.02 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:20:36.19 -32:11:11.1: 11.33 +/- 0.01 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:22:01.12 -32:07:49.4: 11.32 +/- 0.01 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:15:49.85 -31:22:41.0: 11.41 +/- 0.02 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:17:21.02 -30:37:07.1: 11.34 +/- 0.02 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:20:36.19 -32:11:11.1: 11.33 +/- 0.01 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:10:04.11 -33:02:07.6: 11.47 +/- 0.02 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:22:01.12 -32:07:49.4: 11.34 +/- 0.01 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:26:36.10 -34:28:07.3: 11.22 +/- 0.01 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:20:38.78 -32:39:53.3: 11.31 +/- 0.01 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 08:53:22.86 -35:54:14.1: 11.57 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.34 +/- 0.01
Forced photometry filter REJECTED candidate at 09:17:21.02 -30:37:07.1: ref_mag=11.34 +/- 0.01 new_mean_mag=11.2768 delta=0.06 (need > 0.90)
Forced photometry reference-image weighted average: 11.33 +/- 0.01
Forced photometry reference-image weighted average: 11.33 +/- 0.01
Forced photometry reference-image weighted average: 11.23 +/- 0.01
Forced photometry reference-image weighted average: 11.28 +/- 0.01
Forced photometry reference-image weighted average: 11.46 +/- 0.01
Forced photometry filter REJECTED candidate at 09:20:36.19 -32:11:11.1: ref_mag=11.33 +/- 0.01 new_mean_mag=11.2824 delta=0.05 (need > 0.90)
Forced photometry filter REJECTED candidate at 09:22:01.12 -32:07:49.4: ref_mag=11.33 +/- 0.01 new_mean_mag=11.2564 delta=0.07 (need > 0.90)
Forced photometry filter REJECTED candidate at 09:20:38.78 -32:39:53.3: ref_mag=11.28 +/- 0.01 new_mean_mag=11.2910 delta=-0.01 (need > 0.90)
Forced photometry filter REJECTED candidate at 09:26:36.10 -34:28:07.3: ref_mag=11.23 +/- 0.01 new_mean_mag=11.2788 delta=-0.05 (need > 0.90)
Forced photometry filter REJECTED candidate at 09:10:04.11 -33:02:07.6: ref_mag=11.46 +/- 0.01 new_mean_mag=11.2886 delta=0.17 (need > 0.90)
Forced photometry reference-image weighted average: 11.53 +/- 0.02
Forced photometry filter REJECTED candidate at 08:53:22.86 -35:54:14.1: ref_mag=11.53 +/- 0.02 new_mean_mag=11.2936 delta=0.24 (need > 0.90)
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:15:49.85 -31:22:41.0: 11.48 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.44 +/- 0.01
Forced photometry filter REJECTED candidate at 09:15:49.85 -31:22:41.0: ref_mag=11.44 +/- 0.01 new_mean_mag=11.3104 delta=0.13 (need > 0.90)
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:25:59.30 -32:36:21.9: 11.35 +/- 0.02 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:17:23.73 -31:24:42.4: 11.36 +/- 0.02 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:20:56.78 -34:53:00.1: 11.24 +/- 0.01 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:17:02.79 -32:04:35.2: 11.11 +/- 0.01 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-26-35_20.00sec_-4.90C_LIGHT_0094.fits at 09:11:04.45 -33:35:11.2: 10.94 +/- 0.01 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:17:23.73 -31:24:42.4: 11.40 +/- 0.02 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:25:59.30 -32:36:21.9: 11.39 +/- 0.01 detection
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:20:56.78 -34:53:00.1: 11.28 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.38 +/- 0.01
Forced photometry reference-image weighted average: 11.26 +/- 0.01
Forced photometry filter REJECTED candidate at 09:20:56.78 -34:53:00.1: ref_mag=11.26 +/- 0.01 new_mean_mag=11.3011 delta=-0.04 (need > 0.90)
Forced photometry filter REJECTED candidate at 09:17:23.73 -31:24:42.4: ref_mag=11.38 +/- 0.01 new_mean_mag=11.2979 delta=0.08 (need > 0.90)
Forced photometry reference-image weighted average: 11.37 +/- 0.01
Forced photometry filter REJECTED candidate at 09:25:59.30 -32:36:21.9: ref_mag=11.37 +/- 0.01 new_mean_mag=11.3183 delta=0.05 (need > 0.90)
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:17:02.79 -32:04:35.2: 11.14 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.12 +/- 0.01
Forced photometry filter KEPT candidate at 09:17:02.79 -32:04:35.2: ref_mag=11.12 +/- 0.01 new_mean_mag=10.0821 delta=1.04 (need > 0.90)
Forced photometry on wcs_Pyx-02-Q1b1x1_2026-04-08_22-27-30_20.00sec_-4.90C_LIGHT_0095.fits at 09:11:04.45 -33:35:11.2: 10.95 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.95 +/- 0.01
Forced photometry filter KEPT candidate at 09:11:04.45 -33:35:11.2: ref_mag=10.95 +/- 0.01 new_mean_mag=9.9094 delta=1.04 (need > 0.90)
Adding exclusion_list_local.txt__out02951.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04252.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20714.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20730.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 51s
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: 3s
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Considering the candidate 20575_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 20575_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
**** FOUND 09:11:16.12 -30:36:47.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20674_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 20674_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
**** FOUND 09:22:55.34 -30:03:04.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20704_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 20704_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
**** FOUND 08:52:54.54 -29:33:58.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20714_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
Preparing report for the candidate 20714_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
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Considering the candidate 20730_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
Preparing report for the candidate 20730_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
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Considering the candidate 20790_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 20790_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
**** FOUND 09:18:23.53 -32:27:40.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20794_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 20794_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
**** FOUND 09:32:12.46 -36:23:57.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20808_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 20808_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
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Considering the candidate 20816_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 20816_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
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Considering the candidate 20819_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 20819_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
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Considering the candidate 20820_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 20820_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
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Considering the candidate 20823_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 20823_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
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Considering the candidate 20825_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 20825_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
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Considering the candidate 20827_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 20827_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
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Considering the candidate 20830_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 20830_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
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Considering the candidate 20836_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 20836_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
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Considering the candidate 20837_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 20837_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
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Considering the candidate 20839_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 20839_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
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Considering the candidate 20841_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 20841_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
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Considering the candidate 20845_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 20845_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
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Considering the candidate 20846_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 20846_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
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Considering the candidate 20848_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 20848_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
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Considering the candidate 20850_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 20850_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20859_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 20859_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
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Considering the candidate 20861_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 20861_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
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Considering the candidate 20865_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 20865_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
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Considering the candidate 20867_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 20867_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
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Considering the candidate 20869_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 20869_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
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Considering the candidate 20870_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 20870_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20871_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 20871_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20873_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 20873_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20874_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 20874_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
**** FOUND 09:44:12.72 -30:27:42.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20876_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 20876_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
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Considering the candidate 20877_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 20877_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
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Considering the candidate 20878_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 20878_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
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Considering the candidate 20880_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 20880_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20881_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 20881_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
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Considering the candidate 20882_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 20882_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
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Considering the candidate 20884_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 20884_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
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Considering the candidate 20887_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 20887_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
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Considering the candidate 20888_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 20888_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
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Considering the candidate 20890_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 20890_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
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Considering the candidate 20893_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 20893_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
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Considering the candidate 20894_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 20894_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
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Considering the candidate 20896_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 20896_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
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Considering the candidate 20898_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 20898_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
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Considering the candidate 20900_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 20900_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
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Considering the candidate 20901_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 20901_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
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Considering the candidate 20902_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 20902_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
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Considering the candidate 20903_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 20903_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
**** FOUND 09:15:43.96 -34:57:46.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20905_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 20905_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
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Considering the candidate 20906_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 20906_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 20910_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 20910_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
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Considering the candidate 02951_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
Preparing report for the candidate 02951_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
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Considering the candidate 07770_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 07770_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
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Considering the candidate 101453_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 101453_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
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Considering the candidate 101455_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 101455_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
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Considering the candidate 101457_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 101457_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
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Considering the candidate 101458_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 101458_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
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Considering the candidate 101460_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 101460_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101462_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 101462_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101466_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 101466_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101468_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 101468_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101475_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 101475_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
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Considering the candidate 101481_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 101481_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101484_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 101484_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101485_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 101485_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101487_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 101487_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
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Considering the candidate 101493_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 101493_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
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Considering the candidate 101494_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 101494_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
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Considering the candidate 101620_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 101620_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
**** FOUND 08:52:54.55 -29:33:58.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101660_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 101660_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
**** FOUND 09:57:01.16 -35:57:41.1 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 101789_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
Preparing report for the candidate 101789_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
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Considering the candidate 101860_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 101860_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
**** FOUND 09:22:06.30 -29:34:14.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101965_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
Preparing report for the candidate 101965_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
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Considering the candidate 102136_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 102136_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
**** FOUND 08:51:36.36 -28:49:49.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 102171_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
Preparing report for the candidate 102171_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
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Considering the candidate 102327_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
Preparing report for the candidate 102327_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
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Considering the candidate 102328_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 102328_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
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Considering the candidate 102354_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 102354_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
**** FOUND 09:40:22.78 -33:31:21.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 102355_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 102355_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102381_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 102381_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
**** FOUND 09:51:28.50 -38:57:23.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102452_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 102452_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
**** FOUND 08:47:50.36 -31:51:45.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102517_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 102517_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102553_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 102553_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102554_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 102554_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
**** FOUND 09:03:41.93 -34:30:31.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 102661_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
Preparing report for the candidate 102661_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102723_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 102723_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102776_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 102776_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
**** FOUND 08:59:24.70 -29:04:14.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102790_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 102790_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
**** FOUND 09:39:55.14 -39:08:30.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102816_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 102816_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102884_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 102884_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102914_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 102914_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102926_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 102926_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102960_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
Preparing report for the candidate 102960_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102972_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
Preparing report for the candidate 102972_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102978_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 102978_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102980_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 102980_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102989_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 102989_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102991_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 102991_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
**** FOUND 08:49:55.31 -32:44:02.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102999_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 102999_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103001_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 103001_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103011_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 103011_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103021_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 103021_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103023_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 103023_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103033_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
Preparing report for the candidate 103033_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103034_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
Preparing report for the candidate 103034_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103035_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 103035_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103066_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 103066_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103089_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 103089_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103106_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 103106_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103112_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 103112_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103117_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 103117_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103126_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 103126_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103164_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 103164_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103173_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 103173_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103174_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 103174_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103177_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 103177_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103183_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 103183_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103184_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 103184_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103188_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 103188_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103194_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 103194_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103205_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 103205_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103231_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 103231_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103245_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 103245_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103247_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 103247_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103251_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 103251_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103306_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 103306_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103309_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 103309_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103319_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 103319_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103326_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 103326_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103336_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 103336_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103338_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 103338_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103342_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 103342_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103359_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 103359_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103367_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 103367_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103373_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 103373_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103381_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 103381_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103403_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 103403_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103413_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 103413_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103426_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 103426_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
**** FOUND 08:53:25.35 -29:18:48.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103438_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 103438_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103444_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 103444_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103458_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 103458_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103467_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 103467_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103474_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 103474_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103475_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 103475_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103480_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 103480_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103482_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 103482_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103519_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
Preparing report for the candidate 103519_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
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Considering the candidate 103536_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 103536_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
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Considering the candidate 53651_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 53651_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
**** FOUND 09:44:19.72 -38:32:23.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56519_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 56519_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
**** FOUND 08:51:35.20 -36:43:59.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52112_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
Preparing report for the candidate 52112_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
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Considering the candidate 69836_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
Preparing report for the candidate 69836_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
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Considering the candidate 26649_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
Preparing report for the candidate 26649_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
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Considering the candidate 17116_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 17116_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
**** FOUND 09:14:33.35 -31:08:51.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 15634_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
Preparing report for the candidate 15634_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
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Considering the candidate 71427_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
Preparing report for the candidate 71427_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
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Considering the candidate 71337_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
Preparing report for the candidate 71337_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
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Considering the candidate 44500_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
Preparing report for the candidate 44500_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
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Considering the candidate 70067_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
Preparing report for the candidate 70067_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
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Considering the candidate 64719_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
Preparing report for the candidate 64719_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
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Considering the candidate 23019_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
Preparing report for the candidate 23019_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
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Considering the candidate 04911_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 04911_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
Rejecting candidate due to large distance (44.8") between the two second-epoch detections
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Considering the candidate 13290_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 13290_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
**** FOUND 09:44:12.70 -30:27:43.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 65227_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
Preparing report for the candidate 65227_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
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Considering the candidate 58988_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
Preparing report for the candidate 58988_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
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Considering the candidate 44421_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 44421_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
**** FOUND 08:53:33.00 -34:18:56.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67664_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
Preparing report for the candidate 67664_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
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Considering the candidate 26113_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
Preparing report for the candidate 26113_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
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Considering the candidate 59381_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
Preparing report for the candidate 59381_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
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Considering the candidate 09026_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 09026_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
**** FOUND 09:22:55.34 -30:03:04.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 81764_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 81764_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
**** FOUND 09:18:47.02 -35:44:18.1 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 76528_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 76528_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
**** FOUND 09:32:12.46 -36:23:57.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 73895_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
Preparing report for the candidate 73895_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
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Considering the candidate 52686_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
Preparing report for the candidate 52686_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
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Considering the candidate 05790_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 05790_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
**** FOUND 09:16:17.52 -29:36:39.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 46603_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
Preparing report for the candidate 46603_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
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Considering the candidate 24079_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 24079_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
**** FOUND 09:17:02.78 -32:04:35.3 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 70995_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
Preparing report for the candidate 70995_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
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Considering the candidate 64493_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
Preparing report for the candidate 64493_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
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Considering the candidate 24914_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 24914_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
**** FOUND 09:32:40.83 -32:03:03.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 36975_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 36975_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
**** FOUND 09:11:04.45 -33:35:11.1 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 36085_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
Preparing report for the candidate 36085_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
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Considering the candidate 72726_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 72726_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
**** FOUND 09:52:52.61 -36:39:19.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 04012_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 04012_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
**** FOUND 09:27:24.60 -29:27:20.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75622_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
Preparing report for the candidate 75622_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
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Considering the candidate 68840_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 68840_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
**** FOUND 09:40:14.41 -37:22:58.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75981_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
Preparing report for the candidate 75981_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
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Considering the candidate 09329_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
The candidate 09329_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558 did not pass the final checks
**** FOUND 09:51:08.32 -29:53:47.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 43770_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
Preparing report for the candidate 43770_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558
make_report_in_HTML.sh Phase 2 (HTML assembly): 4s
make_report_in_HTML.sh TOTAL: 107s
Prepared the HTML report for the field Pyx-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
09:17:02.79 -32:04:35.2
09:11:04.45 -33:35:11.2
09:18:47.01 -35:44:18.1
09:57:01.14 -35:57:42.2
09:31:04.47 -38:12:21.4
09:31:49.20 -32:26:34.9
09:29:37.12 -36:29:06.3
09:04:28.37 -36:51:09.0
09:17:03.27 -39:03:15.6
09:28:56.61 -38:06:06.3
09:23:45.46 -34:37:21.0
09:52:12.34 -35:36:34.1
08:57:58.51 -35:50:25.1
09:29:17.30 -29:41:41.1
09:20:59.40 -30:56:48.5
09:20:24.96 -31:58:32.7
09:00:07.66 -32:13:05.3
09:26:13.05 -32:18:16.1
09:23:39.86 -33:29:36.3
09:29:56.61 -34:18:20.4
09:39:17.59 -34:19:01.3
09:42:54.37 -34:33:23.4
09:33:02.37 -38:52:40.4
09:28:31.43 -38:50:14.3
09:38:49.66 -35:19:45.5
09:58:21.75 -34:56:55.3
09:13:49.09 -38:07:08.0
09:31:53.73 -38:01:32.5
09:10:02.78 -38:00:19.7
09:05:45.07 -37:39:38.5
09:10:49.66 -37:24:12.8
09:31:23.67 -37:19:58.3
09:14:59.87 -37:15:48.5
09:02:22.40 -37:09:34.4
09:06:33.85 -37:11:06.4
09:13:48.30 -36:52:21.9
09:12:36.29 -36:37:13.3
09:01:08.48 -36:30:30.1
Source monitoring: measuring positions from /data_ssd/NMW-TexasTech/workdir/img_2026-11-03_CI_Pyx-02-Q1b1x1_053531_TTUQ1b1x1_1550823_YDJ5pKlT/monitoring_positions.txt
Source monitoring: positions closer than 100 pix to a frame edge are recorded as edge
Read 54360 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 130.6103 to 150.7018 deg, Dec -39.3523 to -28.1913 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 130.6103 to 150.7018 deg, Dec -39.3523 to -28.1913 deg
Loaded 18251 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): 13233 out of 14365 total matches.
Matched with Tycho-2 14365 out of 54360 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_fd_Pyx-02-Q1b1x1_2026-11-03_05-33-28_20.00sec_-0.00C_LIGHTs_0557.fits via Tycho-2
util/pixel_flux_airmass_correction processing wcs_fd_Pyx-02-Q1b1x1_2026-11-03_05-33-28_20.00sec_-0.00C_LIGHTs_0557.fits
Observation time (mid-exposure, UTC): JD 2461347.98170 (FITS header)
Observing site: lat= +33.748056 deg lon= -101.958333 deg east-positive (SITELAT/SITELONG FITS header keywords)
Frame center (pixel 4788.5 3194.5): RA= 140.84464 deg Dec= -34.00568 deg
Frame center: alt= +17.780 deg az= 152.974 deg airmass= 3.2340
Header cross-check: CENTALT= 17.601 deg (difference +0.179 deg)
Header cross-check: AIRMASS= 3.2747 (we compute 3.2340)
Airmass zero-point fit: OK k= +0.2693 +/- 0.0038 mag/airmass N= 6051 airmass span 2.2929-5.6185 scatter 0.1814 mag
Source monitoring: airmass zero-point for wcs_fd_Pyx-02-Q1b1x1_2026-11-03_05-33-28_20.00sec_-0.00C_LIGHTs_0557.fits: OK +0.941271 -0.269343 3.2340 +0.2693 6051 3.3255 0.1814 2.2929 5.6185
Edge margin: 100.0 pix (FORCED_PHOTOMETRY_EDGE_MARGIN_PIX)
Forced photometry (list mode): image=wcs_fd_Pyx-02-Q1b1x1_2026-11-03_05-33-28_20.00sec_-0.00C_LIGHTs_0557.fits list=monitoring_pixlist1551152.tmp aperture=7.0
Image size: 9576 x 6388
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).
Saturation level: 57000.0
Calibration (from calib.txt_param_monitoring, fit_function=3): cal_mag = 0.000000 * x^2 + 1.000000 * x + 22.584000
Local star coverage test: 54360 stars in wcs_fd_Pyx-02-Q1b1x1_2026-11-03_05-33-28_20.00sec_-0.00C_LIGHTs_0557.fits.wcscat, test radius 301 pix (0.50 deg), 255.7 stars per circle at the frame's mean density
Forced photometry: center=(2378.70, 4034.68) aperture=7.0
Annulus: inner=14.00 outer=35.00 edge margin=100.00
Background annulus: 3233 pixels
Iterative clipping converged after 4 iterations, 3112/3233 pixels remain
SExtractor background: mode=2918.96 median=2925.00 mean=2929.03 sigma=92.17 -> bg=2918.96 (3112 pixels)
Aperture sum=113105.35 N_eff=38.4845
Net flux=770.59 noise=571.77 SNR=1.35
Instrumental magnitude: -8.0858
Calibrated magnitude: 14.4982
Local star coverage at (2378.70, 4034.68): 333 catalog stars within 301 pix, 255.7 expected at the frame's mean star density
Source monitoring: airmass zero-point term applied to the measurements on wcs_fd_Pyx-02-Q1b1x1_2026-11-03_05-33-28_20.00sec_-0.00C_LIGHTs_0557.fits
Source monitoring: 1 position(s) measured on wcs_fd_Pyx-02-Q1b1x1_2026-11-03_05-33-28_20.00sec_-0.00C_LIGHTs_0557.fits (aperture 7.0 pix)
Read 55245 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 130.5761 to 150.7021 deg, Dec -39.3387 to -28.1648 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 130.5761 to 150.7021 deg, Dec -39.3387 to -28.1648 deg
Loaded 18304 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): 13201 out of 14381 total matches.
Matched with Tycho-2 14381 out of 55245 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558.fits via Tycho-2
util/pixel_flux_airmass_correction processing wcs_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558.fits
Observation time (mid-exposure, UTC): JD 2461347.98226 (FITS header)
Observing site: lat= +33.748056 deg lon= -101.958333 deg east-positive (SITELAT/SITELONG FITS header keywords)
Frame center (pixel 4788.5 3194.5): RA= 140.84217 deg Dec= -33.99350 deg
Frame center: alt= +17.858 deg az= 153.154 deg airmass= 3.2208
Header cross-check: CENTALT= 17.728 deg (difference +0.130 deg)
Header cross-check: AIRMASS= 3.2524 (we compute 3.2208)
Airmass zero-point fit: OK k= +0.2778 +/- 0.0037 mag/airmass N= 5982 airmass span 2.2859-5.5368 scatter 0.1778 mag
Source monitoring: airmass zero-point for wcs_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558.fits: OK +0.969384 -0.277816 3.2208 +0.2778 5982 3.2509 0.1778 2.2859 5.5368
Edge margin: 100.0 pix (FORCED_PHOTOMETRY_EDGE_MARGIN_PIX)
Forced photometry (list mode): image=wcs_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558.fits list=monitoring_pixlist1551152.tmp aperture=6.9
Image size: 9576 x 6388
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).
Saturation level: 57000.0
Calibration (from calib.txt_param_monitoring, fit_function=3): cal_mag = 0.000000 * x^2 + 1.000000 * x + 22.576900
Local star coverage test: 55245 stars in wcs_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558.fits.wcscat, test radius 301 pix (0.50 deg), 260.1 stars per circle at the frame's mean density
Forced photometry: center=(2380.12, 4027.22) aperture=6.9
Annulus: inner=13.80 outer=34.50 edge margin=100.00
Background annulus: 3146 pixels
Iterative clipping converged after 5 iterations, 3034/3146 pixels remain
SExtractor background: mode=2912.71 median=2919.00 mean=2923.20 sigma=94.21 -> bg=2912.71 (3034 pixels)
Aperture sum=109968.64 N_eff=37.3928
Net flux=1054.40 noise=576.09 SNR=1.83
Instrumental magnitude: -8.0940
Calibrated magnitude: 14.4829
Local star coverage at (2380.12, 4027.22): 339 catalog stars within 301 pix, 260.1 expected at the frame's mean star density
Source monitoring: airmass zero-point term applied to the measurements on wcs_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558.fits
Source monitoring: 1 position(s) measured on wcs_fd_Pyx-02-Q1b1x1_2026-11-03_05-34-17_20.00sec_0.00C_LIGHTs_0558.fits (aperture 6.9 pix)
########### Completed Pyx-02-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 ####
09:18:47.01 -35:44:18.1
09:57:01.14 -35:57:42.2
09:17:02.79 -32:04:35.2
09:11:04.45 -33:35:11.2
09:31:04.47 -38:12:21.4
09:31:49.20 -32:26:34.9
09:29:37.12 -36:29:06.3
09:04:28.37 -36:51:09.0
09:17:03.27 -39:03:15.6
09:28:56.61 -38:06:06.3
09:23:45.46 -34:37:21.0
09:52:12.34 -35:36:34.1
08:57:58.51 -35:50:25.1
09:29:17.30 -29:41:41.1
09:33:02.37 -38:52:40.4
09:10:49.66 -37:24:12.8
09:26:13.05 -32:18:16.1
09:20:59.40 -30:56:48.5
09:06:33.85 -37:11:06.4
09:02:22.40 -37:09:34.4
09:39:17.59 -34:19:01.3
09:31:23.67 -37:19:58.3
09:31:53.73 -38:01:32.5
09:20:24.96 -31:58:32.7
09:10:02.78 -38:00:19.7
09:38:49.66 -35:19:45.5
09:05:45.07 -37:39:38.5
09:00:07.66 -32:13:05.3
09:58:21.75 -34:56:55.3
09:13:48.30 -36:52:21.9
09:28:31.43 -38:50:14.3
09:42:54.37 -34:33:23.4
09:14:59.87 -37:15:48.5
09:13:49.09 -38:07:08.0
09:23:39.86 -33:29:36.3
09:12:36.29 -36:37:13.3
09:01:08.48 -36:30:30.1
09:29:56.61 -34:18:20.4
###################################################################################
09:18:47.01 -35:44:18.1 -- not an asteroid (will add it to exclusion list)
09:57:01.14 -35:57:42.2 -- not an asteroid (will add it to exclusion list)
09:17:02.79 -32:04:35.2 -- not an asteroid (will add it to exclusion list)
09:11:04.45 -33:35:11.2 -- not an asteroid (will add it to exclusion list)
09:31:04.47 -38:12:21.4 -- not an asteroid (will add it to exclusion list)
09:31:49.20 -32:26:34.9 -- not an asteroid (will add it to exclusion list)
09:29:37.12 -36:29:06.3 -- not an asteroid (will add it to exclusion list)
09:04:28.37 -36:51:09.0 -- not an asteroid (will add it to exclusion list)
09:17:03.27 -39:03:15.6 -- not an asteroid (will add it to exclusion list)
09:28:56.61 -38:06:06.3 -- not an asteroid (will add it to exclusion list)
09:23:45.46 -34:37:21.0 -- not an asteroid (will add it to exclusion list)
09:52:12.34 -35:36:34.1 -- not an asteroid (will add it to exclusion list)
08:57:58.51 -35:50:25.1 -- not an asteroid (will add it to exclusion list)
09:29:17.30 -29:41:41.1 -- not an asteroid (will add it to exclusion list)
09:33:02.37 -38:52:40.4 -- not an asteroid (will add it to exclusion list)
09:10:49.66 -37:24:12.8 -- not an asteroid (will add it to exclusion list)
09:26:13.05 -32:18:16.1 -- not an asteroid (will add it to exclusion list)
09:20:59.40 -30:56:48.5 -- not an asteroid (will add it to exclusion list)
09:06:33.85 -37:11:06.4 -- not an asteroid (will add it to exclusion list)
09:02:22.40 -37:09:34.4 -- not an asteroid (will add it to exclusion list)
09:39:17.59 -34:19:01.3 -- not an asteroid (will add it to exclusion list)
09:31:23.67 -37:19:58.3 -- not an asteroid (will add it to exclusion list)
09:31:53.73 -38:01:32.5 -- not an asteroid (will add it to exclusion list)
09:20:24.96 -31:58:32.7 -- not an asteroid (will add it to exclusion list)
09:10:02.78 -38:00:19.7 -- not an asteroid (will add it to exclusion list)
09:38:49.66 -35:19:45.5 -- not an asteroid (will add it to exclusion list)
09:05:45.07 -37:39:38.5 -- not an asteroid (will add it to exclusion list)
09:00:07.66 -32:13:05.3 -- not an asteroid (will add it to exclusion list)
09:58:21.75 -34:56:55.3 -- not an asteroid (will add it to exclusion list)
09:13:48.30 -36:52:21.9 -- not an asteroid (will add it to exclusion list)
09:28:31.43 -38:50:14.3 -- not an asteroid (will add it to exclusion list)
09:42:54.37 -34:33:23.4 -- not an asteroid (will add it to exclusion list)
09:14:59.87 -37:15:48.5 -- not an asteroid (will add it to exclusion list)
09:13:49.09 -38:07:08.0 -- not an asteroid (will add it to exclusion list)
09:23:39.86 -33:29:36.3 -- not an asteroid (will add it to exclusion list)
09:12:36.29 -36:37:13.3 -- not an asteroid (will add it to exclusion list)
09:01:08.48 -36:30:30.1 -- not an asteroid (will add it to exclusion list)
09:29:56.61 -34:18:20.4 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
08:57:58.51 -35:50:25.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:00:07.66 -32:13:05.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:01:08.48 -36:30:30.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:02:22.40 -37:09:34.4 -- does not seem to be a hot pixel (will add it to exclusion list)
09:04:28.37 -36:51:09.0 -- does not seem to be a hot pixel (will add it to exclusion list)
09:05:45.07 -37:39:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:06:33.85 -37:11:06.4 -- does not seem to be a hot pixel (will add it to exclusion list)
09:10:02.78 -38:00:19.7 -- does not seem to be a hot pixel (will add it to exclusion list)
09:10:49.66 -37:24:12.8 -- does not seem to be a hot pixel (will add it to exclusion list)
09:11:04.45 -33:35:11.2 -- does not seem to be a hot pixel (will add it to exclusion list)
09:12:36.29 -36:37:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:13:48.30 -36:52:21.9 -- does not seem to be a hot pixel (will add it to exclusion list)
09:13:49.09 -38:07:08.0 -- does not seem to be a hot pixel (will add it to exclusion list)
09:14:59.87 -37:15:48.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:17:02.79 -32:04:35.2 -- does not seem to be a hot pixel (will add it to exclusion list)
09:17:03.27 -39:03:15.6 -- does not seem to be a hot pixel (will add it to exclusion list)
09:18:47.01 -35:44:18.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:20:24.96 -31:58:32.7 -- does not seem to be a hot pixel (will add it to exclusion list)
09:20:59.40 -30:56:48.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:23:39.86 -33:29:36.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:23:45.46 -34:37:21.0 -- does not seem to be a hot pixel (will add it to exclusion list)
09:26:13.05 -32:18:16.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:28:31.43 -38:50:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:28:56.61 -38:06:06.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:29:17.30 -29:41:41.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:29:37.12 -36:29:06.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:29:56.61 -34:18:20.4 -- does not seem to be a hot pixel (will add it to exclusion list)
09:31:04.47 -38:12:21.4 -- does not seem to be a hot pixel (will add it to exclusion list)
09:31:23.67 -37:19:58.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:31:49.20 -32:26:34.9 -- does not seem to be a hot pixel (will add it to exclusion list)
09:31:53.73 -38:01:32.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:33:02.37 -38:52:40.4 -- does not seem to be a hot pixel (will add it to exclusion list)
09:38:49.66 -35:19:45.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:39:17.59 -34:19:01.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:42:54.37 -34:33:23.4 -- does not seem to be a hot pixel (will add it to exclusion list)
09:52:12.34 -35:36:34.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:57:01.14 -35:57:42.2 -- does not seem to be a hot pixel (will add it to exclusion list)
09:58:21.75 -34:56:55.3 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
08:57:58.51 -35:50:25.1 -- a known variable star
09:00:07.66 -32:13:05.3 -- a known variable star
09:01:08.48 -36:30:30.1 -- a known variable star
09:02:22.40 -37:09:34.4 -- a known variable star
09:04:28.37 -36:51:09.0 -- a known variable star
09:05:45.07 -37:39:38.5 -- a known variable star
09:06:33.85 -37:11:06.4 -- a known variable star
09:10:02.78 -38:00:19.7 -- a known variable star
09:10:49.66 -37:24:12.8 -- a known variable star
09:11:04.45 -33:35:11.2 -- a known variable star
09:12:36.29 -36:37:13.3 -- a known variable star
09:13:48.30 -36:52:21.9 -- a known variable star
09:13:49.09 -38:07:08.0 -- a known variable star
09:14:59.87 -37:15:48.5 -- a known variable star
09:17:02.79 -32:04:35.2 -- a known variable star
09:17:03.27 -39:03:15.6 -- a known variable star
09:18:47.01 -35:44:18.1 -- a known variable star
09:20:24.96 -31:58:32.7 -- a known variable star
09:20:59.40 -30:56:48.5 -- a known variable star
09:23:39.86 -33:29:36.3 -- a known variable star
09:23:45.46 -34:37:21.0 -- a known variable star
09:26:13.05 -32:18:16.1 -- a known variable star
09:28:31.43 -38:50:14.3 -- a known variable star
09:28:56.61 -38:06:06.3 -- a known variable star
09:29:17.30 -29:41:41.1 -- a known variable star
09:29:37.12 -36:29:06.3 -- a known variable star
09:29:56.61 -34:18:20.4 -- a known variable star
09:31:04.47 -38:12:21.4 -- a known variable star
09:31:23.67 -37:19:58.3 -- a known variable star
09:31:49.20 -32:26:34.9 -- a known variable star
09:31:53.73 -38:01:32.5 -- a known variable star
09:33:02.37 -38:52:40.4 -- a known variable star
09:38:49.66 -35:19:45.5 -- a known variable star
09:39:17.59 -34:19:01.3 -- a known variable star
09:42:54.37 -34:33:23.4 -- a known variable star
09:52:12.34 -35:36:34.1 -- a known variable star
09:57:01.14 -35:57:42.2 -- a known variable star
09:58:21.75 -34:56:55.3 -- a known variable star
Found 0 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
38 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 ####
08:57:58.51 -35:50:25.1
09:00:07.66 -32:13:05.3
09:01:08.48 -36:30:30.1
09:02:22.40 -37:09:34.4
09:04:28.37 -36:51:09.0
09:05:45.07 -37:39:38.5
09:06:33.85 -37:11:06.4
09:10:02.78 -38:00:19.7
09:10:49.66 -37:24:12.8
09:11:04.45 -33:35:11.2
09:12:36.29 -36:37:13.3
09:13:48.30 -36:52:21.9
09:13:49.09 -38:07:08.0
09:14:59.87 -37:15:48.5
09:17:02.79 -32:04:35.2
09:17:03.27 -39:03:15.6
09:18:47.01 -35:44:18.1
09:20:24.96 -31:58:32.7
09:20:59.40 -30:56:48.5
09:23:39.86 -33:29:36.3
09:23:45.46 -34:37:21.0
09:26:13.05 -32:18:16.1
09:28:31.43 -38:50:14.3
09:28:56.61 -38:06:06.3
09:29:17.30 -29:41:41.1
09:29:37.12 -36:29:06.3
09:29:56.61 -34:18:20.4
09:31:04.47 -38:12:21.4
09:31:23.67 -37:19:58.3
09:31:49.20 -32:26:34.9
09:31:53.73 -38:01:32.5
09:33:02.37 -38:52:40.4
09:38:49.66 -35:19:45.5
09:39:17.59 -34:19:01.3
09:42:54.37 -34:33:23.4
09:52:12.34 -35:36:34.1
09:57:01.14 -35:57:42.2
09:58:21.75 -34:56:55.3
####################################################
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461347.98169601 -observatory V36
14:42:18.38 -16:32:26.5 Mercury (5.5mag)
13:25:15.80 -13:32:25.0 Venus (-4.3mag)
09:29:46.05 +16:32:34.4 Mars (0.8mag)
09:47:08.37 +14:05:55.3 Jupiter (-2.0mag)
00:36:23.67 +01:00:28.4 Saturn (0.5mag)
04:09:00.87 +20:50:05.4 Uranus (5.6mag)
00:08:19.52 -00:38:19.7 Neptune (7.7mag)
20:24:28.59 -23:41:31.6 Pluto (14.5mag)
10:15:11.76 +10:11:09.3 Moon (-9.8mag)
-rw-r--r-- 1 apache apache 361 Nov 3 05:40 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461347.98169601:
09:47:01.88 +14:06:33.1 Io (6.0mag)
09:46:59.27 +14:06:48.9 Europa (6.1mag)
09:47:20.53 +14:04:45.7 Ganymede (5.5mag)
09:47:38.16 +14:03:05.6 Callisto (6.8mag)
09:48:35.81 +14:15:21.5 Himalia (15.5mag)
09:47:08.61 +14:05:55.0 Thebe (16.3mag)
09:46:54.69 +14:30:56.3 Elara (17.4mag)
09:47:53.41 +13:33:37.6 Pasiphae (17.7mag)
09:44:09.57 +14:37:50.9 Carme (18.7mag)
00:36:32.89 +01:00:00.5 Titan (8.3mag)
00:36:23.61 +01:00:30.4 Rhea (9.6mag)
00:36:54.17 +01:01:08.4 Iapetus (11.0mag)
00:36:12.76 +01:00:08.0 Hyperion (14.2mag)
00:34:36.94 +00:48:19.1 Phoebe (16.4mag)
-rw-r--r-- 1 apache apache 568 Nov 3 05:40 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461347.98169601:
04:35:14.48 +17:19:26.7 JWST
15:32:51.27 +53:02:21.3 Chandra
07:21:09.20 -22:13:18.4 XMM-Newton
-rw-r--r-- 1 apache apache 96 Nov 3 05:40 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461347.98169601 -observatory V36
03:33:35.71 +19:56:43.1 17.1mag P/1996 R2 (Lagerkvist)
07:46:39.37 +38:23:23.6 17.9mag P/2004 V5 (LINEAR-Hill)
07:46:44.74 +38:23:10.7 17.9mag P/2004 V5-A (LINEAR-Hill)
07:46:03.27 +38:23:30.4 17.9mag P/2004 V5-B (LINEAR-Hill)
05:01:53.23 +39:05:53.9 17.8mag P/2009 Y2 (Kowalski)
18:48:09.51 -32:52:30.4 15.0mag P/2010 H2 (Vales)
07:45:18.30 -73:54:38.5 17.2mag C/2014 UN271 (Bernardinelli-Bernstein)
06:11:27.78 +35:18:38.3 17.7mag C/2017 K2 (PANSTARRS)
07:35:43.08 +25:20:22.4 16.9mag C/2022 N2 (PANSTARRS)
09:08:34.72 +38:32:28.2 16.4mag C/2024 E1 (Wierzchos)
18:37:03.48 +40:52:15.6 17.4mag C/2024 J3 (ATLAS)
05:43:02.13 -13:33:13.1 16.3mag C/2024 T5 (ATLAS)
14:15:21.15 -04:35:35.2 16.3mag C/2025 Y1 (ATLAS)
20:15:02.02 +53:02:24.7 15.2mag C/2026 A2 (Bok)
13:07:39.41 +16:59:45.3 17.7mag A/2026 E1
16:00:27.54 -65:28:08.4 14.5mag P/2026 R2 (Leonard)
19:34:08.24 -05:22:13.3 17.1mag P/2026 T1 (ATLAS)
23:28:44.42 +14:02:24.9 16.8mag 2P/Encke
23:26:09.25 -25:45:22.8 15.4mag 10P/Tempel
02:40:00.76 +30:32:00.4 16.3mag 11P/Tempel-Swift-LINEAR
12:26:12.24 -10:02:30.1 16.3mag 29P/Schwassmann-Wachmann
00:10:39.33 -09:01:17.7 15.9mag 65P/Gunn
08:00:15.38 +13:34:47.2 14.0mag 78P/Gehrels
09:00:01.40 +45:57:58.9 17.1mag 112P/Urata-Niijima
09:51:16.43 +05:34:08.2 17.8mag 114P/Wiseman-Skiff
12:27:01.39 +08:01:51.0 14.8mag 123P/West-Hartley
19:48:47.36 +14:25:51.4 10.2mag 161P/Hartley-IRAS
11:12:19.01 -03:07:11.1 16.2mag 169P/NEAT
09:41:36.32 +23:29:40.7 18.0mag 186P/Garradd
03:10:37.66 +02:10:59.7 15.3mag 220P/McNaught
06:22:38.72 +49:46:55.1 15.6mag 260P/McNaught
07:56:33.15 +25:04:29.4 17.6mag 266P/Christensen
-rw-r--r-- 1 apache apache 1.6K Nov 3 05:40 comets.txt
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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 05:40 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 05:40 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
00:58:27.412 -22:03:24.97 SN 2026afsw 2026-10-17.21 18.226
23:34:39.952 +13:04:33.30 AT 2026afsv 2026-10-18.23 19.8853
01:44:42.847 +02:02:43.85 AT 2026afsu 2026-10-16.33 20.1698
05:01:31.593 +09:22:51.39 AT 2026afst 2026-10-16.48 20.0945
05:07:17.177 +15:10:39.52 AT 2026afss 2026-10-07.48 20.8919
01:46:51.117 -03:32:45.52 AT 2026afsr 2026-10-09.42 20.8495
02:40:13.442 +09:41:35.87 AT 2026afsq 2026-10-09.42 20.8105
01:53:33.220 +15:17:08.15 AT 2026afsp 2026-10-14.33 20.3641
05:17:19.580 -11:56:45.36 AT 2026afso 2026-10-18.42 19.8609
05:07:12.333 -10:39:28.07 AT 2026afsn 2026-10-18.42 19.8368
03:51:59.889 +04:08:13.56 AT 2026afsm 2026-10-18.41 20.0289
10:10:48.919 +25:50:29.45 AT 2026afsl 2026-10-18.53 20.0139
09:28:13.437 -18:47:45.86 AT 2026afsk 2026-10-18.59 18.259
06:18:17.122 +02:53:09.71 AT 2026afsj 2026-10-18.34 19.384
23:15:34.188 -43:11:36.92 AT 2026afsi 2026-10-18.35 18.839
01:05:10.811 +07:14:30.54 SN 2026afsh 2026-10-18.31 18.764
12:02:02.958 +29:50:40.95 SN 2026afsg 2026-10-18.87 16.4
09:23:29.659 +61:32:27.44 AT 2026afsf 2026-09-25.49 19.541
07:38:29.533 +53:56:33.67 AT 2026afse 2026-10-01.41 20.2164
09:06:11.873 +17:26:33.92 AT 2026afsd 2026-10-02.52 19.0664
-rw-r--r-- 1 apache apache 89K Nov 3 05:40 tns_transients_list.txt
