This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-05-Q1b1x1_060151_TTUQ1b1x1_731119_dAowQ001
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 07 12.4249 2461233.9249 10.07 05:33:29.32 +25:28:34.7
181.49959 -4.12273 galactic Tau Second-epoch detections are separated by 3.0" and 9.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3417030801938496640 | 05:33:30.87 +25:28:20.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K2 1931AnHar.100...61C HD 244760
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:33:29.32 +25:28:34.7: 11.23 +/- 0.01 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:33:29.32 +25:28:34.7: 11.21 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.22 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 12.4249* 05 33 29.32 +25 28 34.7 10.1 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3417030801938496640,2461233.9249,10.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3417030801938496640 20260712.4249 10.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4249 2461233.9249 10.13 05:29:33.80 +29:20:53.6
177.77302 -2.73954 galactic Aur Second-epoch detections are separated by 1.8" and 8.9 pix
The object was found in VSX 1" ASASSN-V J052933.91+292054.0
Type: L
# Max. Min./Amp. JD0 Period
12.060 V 13.040 V
The object was not found in astcheck.
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:29:33.80 +29:20:53.6: 11.35 +/- 0.01 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:29:33.80 +29:20:53.6: 11.34 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.34 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J052933.91+292054.0,2461233.9249,10.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J052933.91+292054.0 20260712.4249 10.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4249 2461233.9249 9.38 05:26:51.35 +32:03:07.7
175.19745 -1.72639 galactic Aur Second-epoch detections are separated by 0.1" and 8.8 pix
The object was found in VSX 3" EG Aur
Type: SRB
# Max. Min./Amp. JD0 Period
12.400 pg 13.700 pg 2429710.00000 149.500000000000 : M6.5
The object was not found in astcheck.
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:26:51.35 +32:03:07.7: 10.29 +/- 0.00 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:26:51.35 +32:03:07.7: 10.30 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.30 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
EG Aur,2461233.9249,9.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
EG Aur 20260712.4249 9.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4249 2461233.9249 9.43 05:30:35.40 +32:47:41.9
175.01493 -0.65894 galactic Aur Second-epoch detections are separated by 0.3" and 8.9 pix
The object was found in VSX 2" [D2006] LCG27
Type: SR
# Max. Min./Amp. JD0 Period
12.501 g Y 1.313 g 2458544.22810 180.188992800000 M7
The object was not found in astcheck.
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:30:35.40 +32:47:41.9: 10.63 +/- 0.00 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:30:35.40 +32:47:41.9: 10.64 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.63 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
[D2006] LCG27,2461233.9249,9.43,0.05,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
[D2006] LCG27 20260712.4249 9.43CV 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 07 12.4249 2461233.9249 11.87 04:34:18.76 +30:23:06.6
169.63080 -11.64196 galactic Tau Second-epoch detections are separated by 1.4" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.115 Thyra 0 -1 1 12.2 -0 0
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 04:34:18.76 +30:23:06.6: 16.06 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 04:34:18.76 +30:23:06.6: 16.08 +/- 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 LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 12.4249* 04 34 18.76 +30 23 06.6 11.9 U Tau 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
VARIABLE_NAME,2461233.9249,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260712.4249 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4249 2461233.9249 10.96 05:32:21.08 +25:21:16.9
181.46261 -4.40448 galactic Tau Second-epoch detections are separated by 2.7" and 9.4 pix
The object was found in VSX19" V1409 Tau
Type: EW
# Max. Min./Amp. JD0 Period
10.170 V 10.670 V 2453348.71900 0.307363000000 G5
The object was not found in astcheck.
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:32:21.08 +25:21:16.9: 12.06 +/- 0.01 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:32:21.08 +25:21:16.9: 12.12 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.09 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 12.4249* 05 32 21.08 +25 21 16.9 11.0 U Tau 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
V1409 Tau,2461233.9249,10.96,0.05,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
V1409 Tau 20260712.4249 10.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4249 2461233.9249 11.61 05:28:50.24 +33:29:34.2
174.23044 -0.57993 galactic Aur Second-epoch detections are separated by 0.4" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.89 Julia -0 0 0 11.5 0 0
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:28:50.24 +33:29:34.2: 15.74 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:28:50.24 +33:29:34.2: 15.81 +/- 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 LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461233.9249,11.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260712.4249 11.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4249 2461233.9249 11.26 05:33:05.21 +25:07:43.7
181.74341 -4.38709 galactic Tau Second-epoch detections are separated by 4.8" and 9.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3417006024270312192 | 05:33:06.96 +25:07:28.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:33:05.21 +25:07:43.7: 13.39 +/- 0.04 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:33:05.21 +25:07:43.7: 13.37 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 12.4249* 05 33 05.21 +25 07 43.7 11.3 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3417006024270312192,2461233.9249,11.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3417006024270312192 20260712.4249 11.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4249 2461233.9249 11.41 05:33:32.78 +25:43:15.4
181.30035 -3.97949 galactic Tau Second-epoch detections are separated by 3.9" and 9.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3441104231072494336 | 05:33:34.08 +25:43:04.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:33:32.78 +25:43:15.4: 12.64 +/- 0.02 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:33:32.78 +25:43:15.4: 12.62 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 12.4249* 05 33 32.78 +25 43 15.4 11.4 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3441104231072494336,2461233.9249,11.41,0.05,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
Gaia DR3 3441104231072494336 20260712.4249 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 07 12.4249 2461233.9249 12.07 05:19:44.27 +26:10:31.3
179.19620 -6.31405 galactic Tau Second-epoch detections are separated by 5.7" and 8.7 pix
The object was found in VSX 7" NSVS J0519436+261035
Type: M
# Max. Min./Amp. JD0 Period
11.336 R1 Y 1.769 R1 346.000000000000 M9
The object was not found in astcheck.
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:19:44.27 +26:10:31.3: 15.53 +/- 0.20 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:19:44.27 +26:10:31.3: 15.43 +/- 0.19 detection
Forced photometry reference-image weighted average: 15.48 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 12.4249* 05 19 44.27 +26 10 31.3 12.1 U Tau 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
NSVS J0519436+261035,2461233.9249,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0519436+261035 20260712.4249 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4249 2461233.9249 11.91 05:31:03.09 +24:58:11.2
181.62639 -4.86057 galactic Tau Second-epoch detections are separated by 3.6" and 9.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3416988264582568064 | 05:31:04.31 +24:58:00.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:31:03.09 +24:58:11.2: 12.97 +/- 0.02 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:31:03.09 +24:58:11.2: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 12.4249* 05 31 03.09 +24 58 11.2 11.9 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3416988264582568064,2461233.9249,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3416988264582568064 20260712.4249 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4249 2461233.9249 13.00 04:45:17.75 +31:12:11.8
170.55811 -9.31799 galactic Aur Second-epoch detections are separated by 0.7" and 8.3 pix
The object was found in VSX 1" ASASSN-V J044517.73+311212.8
Type: SR
# Max. Min./Amp. JD0 Period
13.406 r Y 0.580 r 2458366.98330 67.325773000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 04:45:17.75 +31:12:11.8: 13.98 +/- 0.05 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 04:45:17.75 +31:12:11.8: 13.97 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.97 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J044517.73+311212.8,2461233.9249,13.00,0.05,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 J044517.73+311212.8 20260712.4249 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 07 12.4249 2461233.9249 12.18 05:20:40.99 +32:46:02.3
173.87176 -2.39982 galactic Aur Second-epoch detections are separated by 4.1" and 9.0 pix
The object was found in VSX 5" ASASSN-V J052041.33+324605.3
Type: SR
# Max. Min./Amp. JD0 Period
14.620 g Y 0.504 g 2458204.71530 62.873951700000
The object was not found in astcheck.
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:20:40.99 +32:46:02.3: 13.17 +/- 0.03 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:20:40.99 +32:46:02.3: 13.19 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J052041.33+324605.3,2461233.9249,12.18,0.05,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 J052041.33+324605.3 20260712.4249 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4249 2461233.9249 12.41 04:52:40.42 +29:13:59.8
173.12590 -9.32298 galactic Tau Second-epoch detections are separated by 2.1" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J073.1683+29.2334 | 04:52:40.38 +29:14:00.0 (Gaia DR3) | IRR (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.373+/-0.035 (Very red! L if it's a dwarf)
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 04:52:40.42 +29:13:59.8: 13.38 +/- 0.03 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 04:52:40.42 +29:13:59.8: 13.36 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 12.4249* 04 52 40.42 +29 13 59.8 12.4 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J073.1683+29.2334,2461233.9249,12.41,0.05,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
ATO J073.1683+29.2334 20260712.4249 12.41CV 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 07 12.4249 2461233.9249 12.86 05:16:23.38 +31:33:47.1
174.33757 -3.83487 galactic Aur Second-epoch detections are separated by 2.8" and 8.6 pix
The object was found in VSX 2" ASASSN-V J051623.49+313347.9
Type: SR
# Max. Min./Amp. JD0 Period
14.230 V 14.640 V 2457638.10000 61.100000000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:16:23.38 +31:33:47.1: 13.97 +/- 0.05 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:16:23.38 +31:33:47.1: 13.86 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.91 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J051623.49+313347.9,2461233.9249,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J051623.49+313347.9 20260712.4249 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4249 2461233.9249 12.16 05:01:05.18 +32:51:54.4
171.35848 -5.66717 galactic Aur Second-epoch detections are separated by 0.8" and 8.3 pix
The object was found in VSX 1" ASASSN-V J050105.08+325154.9
Type: L
# Max. Min./Amp. JD0 Period
13.090 V 13.610 V
The object was not found in astcheck.
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:01:05.18 +32:51:54.4: 13.06 +/- 0.02 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:01:05.18 +32:51:54.4: 13.10 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J050105.08+325154.9,2461233.9249,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J050105.08+325154.9 20260712.4249 12.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4249 2461233.9249 12.71 04:59:57.74 +27:26:58.9
175.54945 -9.14842 galactic Tau Second-epoch detections are separated by 2.1" and 8.4 pix
The object was found in VSX 1" ASASSN-V J045957.69+272659.2
Type: L
# Max. Min./Amp. JD0 Period
13.960 V 14.280 V
The object was not found in astcheck.
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 04:59:57.74 +27:26:58.9: 13.64 +/- 0.03 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 04:59:57.74 +27:26:58.9: 13.69 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 12.4249* 04 59 57.74 +27 26 58.9 12.7 U Tau 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 J045957.69+272659.2,2461233.9249,12.71,0.05,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 J045957.69+272659.2 20260712.4249 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4249 2461233.9249 11.42 05:20:58.54 +25:08:44.2
180.21045 -6.66424 galactic Tau Second-epoch detections are separated by 1.1" and 9.1 pix
The object was found in VSX 5" ASAS J052059+2508.7
Type: MISC
# Max. Min./Amp. JD0 Period
13.160 V Y 0.580 V 2453248.20000 240.956167000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:20:58.54 +25:08:44.2: 12.40 +/- 0.01 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:20:58.54 +25:08:44.2: 12.45 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.42 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 12.4249* 05 20 58.54 +25 08 44.2 11.4 U Tau 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 J052059+2508.7,2461233.9249,11.42,0.05,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 J052059+2508.7 20260712.4249 11.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4249 2461233.9249 12.84 05:12:02.91 +32:26:56.3
173.07851 -4.06734 galactic Aur Second-epoch detections are separated by 3.1" and 9.0 pix
The object was found in VSX 1" ASASSN-V J051202.88+322656.7
Type: SR
# Max. Min./Amp. JD0 Period
14.570 V 15.370 V 2458444.24110 194.080141400000
The object was not found in astcheck.
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:12:02.91 +32:26:56.3: 13.86 +/- 0.04 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:12:02.91 +32:26:56.3: 13.87 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.86 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J051202.88+322656.7,2461233.9249,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J051202.88+322656.7 20260712.4249 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4249 2461233.9249 12.41 05:05:08.99 +25:22:10.4
177.94296 -9.45950 galactic Tau Second-epoch detections are separated by 0.7" and 8.6 pix
The object was found in VSX 2" NSVS J0505090+252211
Type: L:
# Max. Min./Amp. JD0 Period
11.448 R1 Y 0.482 R1 277.000000000000 M7
The object was not found in astcheck.
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:05:08.99 +25:22:10.4: 13.64 +/- 0.04 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:05:08.99 +25:22:10.4: 13.59 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 12.4249* 05 05 08.99 +25 22 10.4 12.4 U Tau 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
NSVS J0505090+252211,2461233.9249,12.41,0.05,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
NSVS J0505090+252211 20260712.4249 12.41CV 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 07 12.4249 2461233.9249 12.53 04:45:50.66 +28:10:28.4
173.00947 -11.15333 galactic Tau Second-epoch detections are separated by 1.4" and 8.6 pix
The object was found in VSX 0" ASASSN-V J044550.66+281028.3
Type: SR
# Max. Min./Amp. JD0 Period
14.220 V 14.580 V 2458505.87050 92.733309000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 04:45:50.66 +28:10:28.4: 13.61 +/- 0.03 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 04:45:50.66 +28:10:28.4: 13.64 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 12.4249* 04 45 50.66 +28 10 28.4 12.5 U Tau 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 J044550.66+281028.3,2461233.9249,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J044550.66+281028.3 20260712.4249 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4249 2461233.9249 12.92 04:58:45.63 +32:09:05.0
171.62473 -6.49163 galactic Aur Second-epoch detections are separated by 2.6" and 8.1 pix
The object was found in VSX 1" ASASSN-V J045845.70+320905.0
Type: SR
# Max. Min./Amp. JD0 Period
13.960 V 14.240 V 2458511.64570 30.034071000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 04:58:45.63 +32:09:05.0: 13.86 +/- 0.04 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 04:58:45.63 +32:09:05.0: 13.96 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.91 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J045845.70+320905.0,2461233.9249,12.92,0.05,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 J045845.70+320905.0 20260712.4249 12.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4249 2461233.9249 11.36 05:08:43.29 +26:03:10.8
177.86220 -8.40691 galactic Tau Second-epoch detections are separated by 0.9" and 8.6 pix
The object was found in VSX 0" NSVS 6898797
Type: L
# Max. Min./Amp. JD0 Period
10.450 R1 10.700 R1
The object was not found in astcheck.
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:08:43.29 +26:03:10.8: 12.29 +/- 0.01 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:08:43.29 +26:03:10.8: 12.31 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.30 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 12.4249* 05 08 43.29 +26 03 10.8 11.4 U Tau 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
NSVS 6898797,2461233.9249,11.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 6898797 20260712.4249 11.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4249 2461233.9249 11.53 05:07:35.82 +29:00:15.8
175.30695 -6.87090 galactic Aur Second-epoch detections are separated by 1.8" and 8.4 pix
The object was found in VSX 1" PR Aur
Type: SRB
# Max. Min./Amp. JD0 Period
14.900 pg 15.600 pg 57.400000000000 M6
The object was not found in astcheck.
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:07:35.82 +29:00:15.8: 12.81 +/- 0.02 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:07:35.82 +29:00:15.8: 12.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
PR Aur,2461233.9249,11.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
PR Aur 20260712.4249 11.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4249 2461233.9249 12.01 05:06:29.74 +29:26:30.7
174.80868 -6.80477 galactic Aur Second-epoch detections are separated by 0.5" and 8.6 pix
The object was found in VSX 0" V0475 Aur
Type: SR:
# Max. Min./Amp. JD0 Period
13.800 pg 14.900 pg 211.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:06:29.74 +29:26:30.7: 13.03 +/- 0.02 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:06:29.74 +29:26:30.7: 13.05 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0475 Aur,2461233.9249,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0475 Aur 20260712.4249 12.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4249 2461233.9249 11.25 04:53:30.35 +31:26:31.6
171.49052 -7.80765 galactic Aur Second-epoch detections are separated by 0.3" and 8.3 pix
The object was found in VSX13" ASASSN-V J045331.38+312632.1
Type: SR
# Max. Min./Amp. JD0 Period
12.650 V 13.260 V 2457607.10000 84.500000000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 04:53:30.35 +31:26:31.6: 12.26 +/- 0.01 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 04:53:30.35 +31:26:31.6: 12.26 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.26 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J045331.38+312632.1,2461233.9249,11.25,0.05,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 J045331.38+312632.1 20260712.4249 11.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4249 2461233.9249 12.66 05:05:51.08 +26:46:29.3
176.88986 -8.50160 galactic Tau Second-epoch detections are separated by 1.9" and 8.6 pix
The object was found in VSX 1" ASASSN-V J050551.05+264629.9
Type: L
# Max. Min./Amp. JD0 Period
14.130 V 14.470 V
The object was not found in astcheck.
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:05:51.08 +26:46:29.3: 13.81 +/- 0.04 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:05:51.08 +26:46:29.3: 13.72 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.76 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 12.4249* 05 05 51.08 +26 46 29.3 12.7 U Tau 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 J050551.05+264629.9,2461233.9249,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J050551.05+264629.9 20260712.4249 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4249 2461233.9249 11.77 05:02:50.79 +28:43:15.6
174.91092 -7.87481 galactic Aur Second-epoch detections are separated by 1.6" and 8.5 pix
The object was found in VSX 1" ASASSN-V J050250.83+284316.0
Type: L
# Max. Min./Amp. JD0 Period
13.190 V 13.610 V
The object was not found in astcheck.
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:02:50.79 +28:43:15.6: 12.78 +/- 0.01 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:02:50.79 +28:43:15.6: 12.72 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.75 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J050250.83+284316.0,2461233.9249,11.77,0.05,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 J050250.83+284316.0 20260712.4249 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4249 2461233.9249 11.28 05:06:18.62 +28:34:06.1
175.49236 -7.35643 galactic Tau Second-epoch detections are separated by 0.4" and 8.7 pix
The object was found in VSX 1" ASASSN-V J050618.63+283406.8
Type: SR
# Max. Min./Amp. JD0 Period
12.580 V 12.970 V 2457447.80000 50.300000000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:06:18.62 +28:34:06.1: 12.20 +/- 0.01 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:06:18.62 +28:34:06.1: 12.17 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.19 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 12.4249* 05 06 18.62 +28 34 06.1 11.3 U Tau 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 J050618.63+283406.8,2461233.9249,11.28,0.05,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 J050618.63+283406.8 20260712.4249 11.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4249 2461233.9249 12.61 05:01:21.17 +30:48:07.8
173.04058 -6.87686 galactic Aur Second-epoch detections are separated by 2.7" and 8.4 pix
The object was found in VSX 1" ZTF J050121.11+304808.1
Type: SR
# Max. Min./Amp. JD0 Period
15.338 g Y 0.600 g 2458378.12400 85.881463100000
The object was not found in astcheck.
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:01:21.17 +30:48:07.8: 13.79 +/- 0.04 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:01:21.17 +30:48:07.8: 13.82 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J050121.11+304808.1,2461233.9249,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J050121.11+304808.1 20260712.4249 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4249 2461233.9249 13.27 04:59:02.06 +31:50:19.3
171.90922 -6.63748 galactic Aur Second-epoch detections are separated by 1.7" and 8.7 pix
The object was found in VSX 1" NSVS J0459027+315024
Type: SRA
# Max. Min./Amp. JD0 Period
16.299 g Y 1.880 g 2458285.49690 411.268265900000 C
The object was not found in astcheck.
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 04:59:02.06 +31:50:19.3: 14.93 +/- 0.11 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 04:59:02.06 +31:50:19.3: 15.18 +/- 0.14 detection
Forced photometry reference-image weighted average: 15.02 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0459027+315024,2461233.9249,13.27,0.05,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
NSVS J0459027+315024 20260712.4249 13.27CV 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 07 12.4249 2461233.9249 12.49 05:18:31.28 +27:01:53.9
178.33173 -6.05230 galactic Tau Second-epoch detections are separated by 4.7" and 8.6 pix
The object was found in VSX 2" ASASSN-V J051831.19+270155.5
Type: SR
# Max. Min./Amp. JD0 Period
15.250 g Y 0.450 g 2459433.94000 32.120000000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:18:31.28 +27:01:53.9: 13.53 +/- 0.03 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:18:31.28 +27:01:53.9: 13.54 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.54 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 12.4249* 05 18 31.28 +27 01 53.9 12.5 U Tau 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 J051831.19+270155.5,2461233.9249,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J051831.19+270155.5 20260712.4249 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4249 2461233.9249 12.00 04:38:07.76 +29:58:31.9
170.49848 -11.28836 galactic Tau Second-epoch detections are separated by 1.4" and 8.3 pix
The object was found in VSX13" NSVS J0438085+295823
Type: L:
# Max. Min./Amp. JD0 Period
11.027 R1 Y 0.407 R1 217.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 04:38:07.76 +29:58:31.9: 12.93 +/- 0.02 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 04:38:07.76 +29:58:31.9: 12.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 12.4249* 04 38 07.76 +29 58 31.9 12.0 U Tau 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
NSVS J0438085+295823,2461233.9249,12.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0438085+295823 20260712.4249 12.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4249 2461233.9249 12.66 05:06:14.13 +32:02:13.4
172.68055 -5.30149 galactic Aur Second-epoch detections are separated by 4.0" and 9.1 pix
The object was found in VSX 1" ASASSN-V J050614.08+320212.2
Type: SR
# Max. Min./Amp. JD0 Period
12.798 r Y 0.875 r 2458334.50630 372.470172400000
The object was not found in astcheck.
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:06:14.13 +32:02:13.4: 13.70 +/- 0.03 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:06:14.13 +32:02:13.4: 13.73 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.72 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J050614.08+320212.2,2461233.9249,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J050614.08+320212.2 20260712.4249 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4249 2461233.9249 11.63 05:18:54.39 +25:01:24.8
180.04597 -7.12001 galactic Tau Second-epoch detections are separated by 1.4" and 9.2 pix
The object was found in VSX 7" NSVS J0518547+250122
Type: SR
# Max. Min./Amp. JD0 Period
14.777 g Y 0.544 g 2458472.96820 206.916780700000
The object was not found in astcheck.
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:18:54.39 +25:01:24.8: 12.65 +/- 0.02 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:18:54.39 +25:01:24.8: 12.69 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 12.4249* 05 18 54.39 +25 01 24.8 11.6 U Tau 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
NSVS J0518547+250122,2461233.9249,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0518547+250122 20260712.4249 11.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4249 2461233.9249 12.17 05:22:54.04 +27:26:39.4
178.54240 -5.01603 galactic Tau Second-epoch detections are separated by 3.1" and 8.4 pix
The object was found in VSX 5" NSVS J0522536+272642
Type: L:
# Max. Min./Amp. JD0 Period
11.021 R1 Y 0.451 R1 145.000000000000 M6
The object was not found in astcheck.
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:22:54.04 +27:26:39.4: 13.32 +/- 0.03 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:22:54.04 +27:26:39.4: 13.32 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 12.4249* 05 22 54.04 +27 26 39.4 12.2 U Tau 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
NSVS J0522536+272642,2461233.9249,12.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0522536+272642 20260712.4249 12.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4249 2461233.9249 12.86 04:51:12.37 +25:58:31.7
175.52121 -11.59704 galactic Tau Second-epoch detections are separated by 4.6" and 9.3 pix
The object was found in VSX 2" ASASSN-V J045112.26+255829.9
Type: L:
# Max. Min./Amp. JD0 Period
15.300 V 15.800 V
The object was not found in astcheck.
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 04:51:12.37 +25:58:31.7: 14.51 +/- 0.08 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 04:51:12.37 +25:58:31.7: 14.34 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.41 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 12.4249* 04 51 12.37 +25 58 31.7 12.9 U Tau 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 J045112.26+255829.9,2461233.9249,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J045112.26+255829.9 20260712.4249 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4249 2461233.9249 12.91 05:01:11.29 +32:26:10.7
171.71336 -5.91145 galactic Aur Second-epoch detections are separated by 1.9" and 8.4 pix
The object was found in VSX 1" NSVS J0501114+322616
Type: SR
# Max. Min./Amp. JD0 Period
13.478 r Y 0.741 r 2458346.43770 234.789576900000
The object was not found in astcheck.
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:01:11.29 +32:26:10.7: 14.31 +/- 0.06 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:01:11.29 +32:26:10.7: 14.36 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.33 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0501114+322616,2461233.9249,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0501114+322616 20260712.4249 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4249 2461233.9249 11.54 05:25:49.97 +30:05:45.3
176.70040 -2.99912 galactic Aur Second-epoch detections are separated by 2.2" and 8.8 pix
The object was found in VSX 1" ASASSN-V J052550.01+300546.4
Type: SR
# Max. Min./Amp. JD0 Period
12.940 V 13.890 V 2458207.41950 89.404574100000
The object was not found in astcheck.
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:25:49.97 +30:05:45.3: 12.59 +/- 0.02 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:25:49.97 +30:05:45.3: 12.65 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J052550.01+300546.4,2461233.9249,11.54,0.05,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 J052550.01+300546.4 20260712.4249 11.54CV 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 07 12.4249 2461233.9249 12.27 05:02:27.13 +32:51:56.9
171.53320 -5.43909 galactic Aur Second-epoch detections are separated by 0.6" and 8.4 pix
The object was found in VSX 1" ASASSN-V J050227.07+325157.5
Type: SR
# Max. Min./Amp. JD0 Period
13.390 V 13.910 V 2457806.80000 825.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:02:27.13 +32:51:56.9: 13.24 +/- 0.02 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:02:27.13 +32:51:56.9: 13.27 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.25 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J050227.07+325157.5,2461233.9249,12.27,0.05,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 J050227.07+325157.5 20260712.4249 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 07 12.4249 2461233.9249 11.55 05:07:49.51 +30:24:04.3
174.20427 -6.00318 galactic Aur Second-epoch detections are separated by 0.7" and 8.6 pix
The object was found in VSX 1" RW Aur
Type: CTTS/ROT+
# Max. Min./Amp. JD0 Period
9.200 V 13.600 V 2.640000000000 K1-K4+K5
The object was not found in astcheck.
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:07:49.51 +30:24:04.3: 12.52 +/- 0.01 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:07:49.51 +30:24:04.3: 12.50 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.51 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
RW Aur,2461233.9249,11.55,0.05,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
RW Aur 20260712.4249 11.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4249 2461233.9249 11.36 05:06:16.52 +27:22:15.4
176.46077 -8.07264 galactic Tau Second-epoch detections are separated by 0.3" and 8.6 pix
The object was found in VSX 1" AR Tau
Type: SR
# Max. Min./Amp. JD0 Period
13.080 V Y 1.120 V 2452622.55000 130.000000000000 :
The object was not found in astcheck.
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:06:16.52 +27:22:15.4: 12.52 +/- 0.01 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:06:16.52 +27:22:15.4: 12.52 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.52 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 12.4249* 05 06 16.52 +27 22 15.4 11.4 U Tau 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
AR Tau,2461233.9249,11.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
AR Tau 20260712.4249 11.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4249 2461233.9249 13.17 05:05:26.34 +31:29:49.7
173.01315 -5.76038 galactic Aur Second-epoch detections are separated by 3.1" and 8.8 pix
The object was found in VSX 3" ASASSN-V J050526.09+312949.9
Type: SR
# Max. Min./Amp. JD0 Period
15.760 g Y 0.900 g 2459503.97500 73.690000000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:05:26.34 +31:29:49.7: 14.31 +/- 0.06 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:05:26.34 +31:29:49.7: 14.25 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.28 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J050526.09+312949.9,2461233.9249,13.17,0.05,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 J050526.09+312949.9 20260712.4249 13.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4249 2461233.9249 11.40 05:33:23.04 +29:29:45.3
178.10485 -1.96232 galactic Aur Second-epoch detections are separated by 1.7" and 8.8 pix
The object was found in VSX 4" NSVS 6926592
Type: SR
# Max. Min./Amp. JD0 Period
15.247 g Y 0.805 g 2458477.47350 154.063864800000 M6
The object was not found in astcheck.
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:33:23.04 +29:29:45.3: 12.46 +/- 0.01 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:33:23.04 +29:29:45.3: 12.50 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.48 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 6926592,2461233.9249,11.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 6926592 20260712.4249 11.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4249 2461233.9249 11.32 05:13:59.20 +31:03:18.6
174.45421 -4.54753 galactic Aur Second-epoch detections are separated by 1.4" and 8.4 pix
The object was found in VSX 1" ASASSN-V J051359.17+310319.3
Type: SR
# Max. Min./Amp. JD0 Period
12.390 V 12.810 V 2458561.68510 86.588815800000
The object was not found in astcheck.
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:13:59.20 +31:03:18.6: 12.41 +/- 0.01 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:13:59.20 +31:03:18.6: 12.44 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.42 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J051359.17+310319.3,2461233.9249,11.32,0.05,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 J051359.17+310319.3 20260712.4249 11.32CV 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.80049318 23.12.2025 07:12:32.611 /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
First image: 2461032.80049318 23.12.2025 07:12:32.611 /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
Last image: 2461233.92519919 12.07.2026 10:12:07.210 /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-05-Q1b1x1_060151_TTUQ1b1x1_731119_dAowQ001/fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 42
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.59
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: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 15212
Objects passed selection criteria: 15097
Measurements per detected object (mean, median, min, max): 2.5 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.5 2.0 2 4
Average stars detected per image: 9972.5
Average stars matched: 9656.75 (96.8338 %)
Memory usage VmPeak: 123488 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sat Jul 11 21:08:03 CDT 2026
VaST build number 1.0rc89-146-gb95cfcf3
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Jul 12 07:40:51 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.80049318 23.12.2025 07:12:32.611 /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
First image: 2461032.80049318 23.12.2025 07:12:32.611 /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
Last image: 2461233.92519919 12.07.2026 10:12:07.210 /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-05-Q1b1x1_060151_TTUQ1b1x1_731119_dAowQ001/fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.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.: -7.27
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: 25 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 116517
Objects passed selection criteria: 116206
Measurements per detected object (mean, median, min, max): 2.5 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.5 2.0 2 4
Average stars detected per image: 78143.2
Average stars matched: 74772.5 (95.6864 %)
Memory usage VmPeak: 1886188 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sat Jul 11 21:08:03 CDT 2026
VaST build number 1.0rc89-146-gb95cfcf3
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Jul 12 07:44:47 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-05-Q1b1x1_060151_TTUQ1b1x1_731119_dAowQ001/fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-05-Q1b1x1_060151_TTUQ1b1x1_731119_dAowQ001/fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits
SExtractor catalog cache: saved Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat to cache
SExtractor catalog cache: saved Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.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/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-05-Q1b1x1_060151_TTUQ1b1x1_731119_dAowQ001/fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-05-Q1b1x1_060151_TTUQ1b1x1_731119_dAowQ001/fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.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: 2461233.92456365
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_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits exists and is non-empty
Saving wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits to local_wcs_cache/
'wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits' -> 'local_wcs_cache/wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits'
wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits exists and is non-empty
Saving wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits to local_wcs_cache/
'wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits' -> 'local_wcs_cache/wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits'
wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits exists and is non-empty
Saving wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits to local_wcs_cache/
'wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits' -> 'local_wcs_cache/wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits'
wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits exists and is non-empty
Saving wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits to local_wcs_cache/
'wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits' -> 'local_wcs_cache/wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits (1st reference image)
verification OK: wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
Image size: 941.5'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:00:01.017 +29:59:40.48 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits (1st new image)
verification OK: wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits
Image size: 946.9'x627.0' 15.8(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.93"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:00:08.249 +30:02:21.77 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:00:01.017 +29:59:40.48
Second-epoch image center 05:00:08.249 +30:02:21.77
Angular distance between the image centers 0.0518 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits (2nd new image)
verification OK: wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits
Image size: 946.7'x627.0' 15.8(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.93"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:00:05.711 +30:01:43.41 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:00:01.017 +29:59:40.48
Second-epoch image center 05:00:05.711 +30:01:43.41
Angular distance between the image centers 0.0381 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 05:00:08.249 +30:02:21.77
Second-epoch second image center 05:00:05.711 +30:01:43.41
Angular distance between the image centers 0.01405 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/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits &> /tmp/tmp.Lv8uDgc7yv
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits &> /tmp/tmp.AKwOVSkMlb
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-05-Q1b1x1_060151_TTUQ1b1x1_731119_dAowQ001/fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits &> /tmp/tmp.Da3C9Hntcj
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-05-Q1b1x1_060151_TTUQ1b1x1_731119_dAowQ001/fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-05-Q1b1x1_060151_TTUQ1b1x1_731119_dAowQ001/fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits &> /tmp/tmp.WBybW0KiCi
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-05-Q1b1x1_060151_TTUQ1b1x1_731119_dAowQ001/fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.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_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits and wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.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_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits and wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat
Found non-empty wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits and wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat
The reference image (wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits) and catalog (wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat) found
'wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat' -> 'wcsmag.cat'
Read 16295 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 65.5643 to 84.6645 deg, Dec +24.3655 to +35.2867 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 65.5643 to 84.6645 deg, Dec 24.3655 to 35.2867 deg
Loaded 8424 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): 6043 out of 6742 total matches.
Matched with Tycho-2 6742 out of 16295 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.988200
a=0.000000 b=1.000000 c=22.988200
From vast_summary.log: estimated ref. image limiting mag.: -7.59
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.40
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.40
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 16295 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 65.5643 to 84.6645 deg, Dec +24.3655 to +35.2867 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 65.5643 to 84.6645 deg, Dec 24.3655 to 35.2867 deg
Loaded 8424 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): 6043 out of 6742 total matches.
Matched with Tycho-2 6742 out of 16295 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits:
Forced-photometry filter: calibrated wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits -> calib.txt_param_ref_wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits (aperture=6.0)
Read 16349 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 65.5645 to 84.6680 deg, Dec +24.3653 to +35.2868 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 65.5645 to 84.6680 deg, Dec 24.3653 to 35.2868 deg
Loaded 8428 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): 6047 out of 6745 total matches.
Matched with Tycho-2 6745 out of 16349 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits:
Forced-photometry filter: calibrated wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits -> calib.txt_param_ref_wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits (aperture=6.0)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 35 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
1.9 pix Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
1.9 pix Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
3.0 pix fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits
3.0 pix fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits
1.9 pix wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
1.9 pix wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
Limiting magnitude estimates:
15.4 mag. Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
15.4 mag. Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
13.1 mag. fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits
13.1 mag. fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits
All-image limiting magnitude estimate: 13.1 (SNR ) 10.9 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.Lv8uDgc7yv (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-12_CI_Aur-05-Q1b1x1_060151_TTUQ1b1x1_731119_dAowQ001/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits' -> 'wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
WCS_IMAGE_NAME=wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
WCS-calibrated image found: wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
Checking if the catalog wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat corresponding to the image wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits alredy exist and is non-empty...
Catalog wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat corresponding to the image wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
WCS catalog name: wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.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=1498, bad_region=0, passed=16295
Got 16295 stars (including 14768 good ones) from the SExtractor catalog wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat
util/solve_plate_with_UCAC5 got 16295 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
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 928 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 15808 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 15809 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 15809 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 954 stars left (next iteration limit 1049)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits N_match=954 sigma_overall_arcsec=0.376 sigma_q1_arcsec=0.403 sigma_q2_arcsec=0.379 sigma_q3_arcsec=0.357 sigma_q4_arcsec=0.320 n_q1=360 n_q2=220 n_q3=212 n_q4=162 worst_quadrant_to_overall_ratio=1.070
The image catalog is written to wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits -region wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.AKwOVSkMlb (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-12_CI_Aur-05-Q1b1x1_060151_TTUQ1b1x1_731119_dAowQ001/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits' -> 'wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
WCS_IMAGE_NAME=wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
WCS-calibrated image found: wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
Checking if the catalog wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.wcscat corresponding to the image wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits alredy exist and is non-empty...
Catalog wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.wcscat corresponding to the image wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
WCS catalog name: wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.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=1486, bad_region=0, passed=16349
Got 16349 stars (including 14839 good ones) from the SExtractor catalog wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.wcscat
util/solve_plate_with_UCAC5 got 16349 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
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 928 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 15776 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 15778 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 15778 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 954 stars left (next iteration limit 1049)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits N_match=954 sigma_overall_arcsec=0.374 sigma_q1_arcsec=0.437 sigma_q2_arcsec=0.357 sigma_q3_arcsec=0.315 sigma_q4_arcsec=0.280 n_q1=362 n_q2=224 n_q3=203 n_q4=165 worst_quadrant_to_overall_ratio=1.168
The image catalog is written to wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits -region wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.Da3C9Hntcj (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-12_CI_Aur-05-Q1b1x1_060151_TTUQ1b1x1_731119_dAowQ001/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-05-Q1b1x1_060151_TTUQ1b1x1_731119_dAowQ001/fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-05-Q1b1x1_060151_TTUQ1b1x1_731119_dAowQ001/fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-05-Q1b1x1_060151_TTUQ1b1x1_731119_dAowQ001/fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-05-Q1b1x1_060151_TTUQ1b1x1_731119_dAowQ001/fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-05-Q1b1x1_060151_TTUQ1b1x1_731119_dAowQ001/fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-05-Q1b1x1_060151_TTUQ1b1x1_731119_dAowQ001/fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits
WCS_IMAGE_NAME=wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits
WCS-calibrated image found: wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits
Checking if the catalog wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits.wcscat corresponding to the image wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits.wcscat corresponding to the image wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-05-Q1b1x1_060151_TTUQ1b1x1_731119_dAowQ001/fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits
WCS catalog name: wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.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=171, bad_region=0, passed=3774
Got 3774 stars (including 3597 good ones) from the SExtractor catalog wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits.wcscat
util/solve_plate_with_UCAC5 got 3774 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 946.9'
Seting catalog search parameters based on the expected field of view 946.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013151 (47.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010521 (37.9 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 629 (Dec 24.2 to 35.5)
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 902 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 3579 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 629 (Dec 24.2 to 35.5)
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 3580 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 3580 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Excluding outliers - 933 stars left (next iteration limit 1026)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits N_match=933 sigma_overall_arcsec=0.589 sigma_q1_arcsec=0.554 sigma_q2_arcsec=0.900 sigma_q3_arcsec=0.513 sigma_q4_arcsec=0.629 n_q1=169 n_q2=119 n_q3=295 n_q4=350 worst_quadrant_to_overall_ratio=1.527
The image catalog is written to wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-05-Q1b1x1_060151_TTUQ1b1x1_731119_dAowQ001/fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits -region wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.WBybW0KiCi (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-12_CI_Aur-05-Q1b1x1_060151_TTUQ1b1x1_731119_dAowQ001/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-05-Q1b1x1_060151_TTUQ1b1x1_731119_dAowQ001/fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-05-Q1b1x1_060151_TTUQ1b1x1_731119_dAowQ001/fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-05-Q1b1x1_060151_TTUQ1b1x1_731119_dAowQ001/fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-05-Q1b1x1_060151_TTUQ1b1x1_731119_dAowQ001/fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-05-Q1b1x1_060151_TTUQ1b1x1_731119_dAowQ001/fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-05-Q1b1x1_060151_TTUQ1b1x1_731119_dAowQ001/fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits
WCS_IMAGE_NAME=wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits
WCS-calibrated image found: wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits
Checking if the catalog wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits.wcscat corresponding to the image wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits.wcscat corresponding to the image wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-05-Q1b1x1_060151_TTUQ1b1x1_731119_dAowQ001/fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits
WCS catalog name: wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.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=153, bad_region=0, passed=3774
Got 3774 stars (including 3619 good ones) from the SExtractor catalog wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits.wcscat
util/solve_plate_with_UCAC5 got 3774 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 946.7'
Seting catalog search parameters based on the expected field of view 946.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013149 (47.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010519 (37.9 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 629 (Dec 24.2 to 35.4)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 905 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 3581 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 629 (Dec 24.2 to 35.4)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 3581 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 3581 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Excluding outliers - 935 stars left (next iteration limit 1028)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits N_match=935 sigma_overall_arcsec=0.614 sigma_q1_arcsec=0.642 sigma_q2_arcsec=0.818 sigma_q3_arcsec=0.522 sigma_q4_arcsec=0.626 n_q1=168 n_q2=121 n_q3=294 n_q4=352 worst_quadrant_to_overall_ratio=1.333
The image catalog is written to wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-05-Q1b1x1_060151_TTUQ1b1x1_731119_dAowQ001/fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits -region wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits sigma_overall=0.376 worst_q_ratio=1.070
ref2=Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits sigma_overall=0.374 worst_q_ratio=1.168
new1=fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits sigma_overall=0.589 worst_q_ratio=1.527
new2=fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits sigma_overall=0.614 worst_q_ratio=1.333
reference average sigma_overall=0.375 worst_q_ratio=1.119
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362_astrometric_residuals.png (954 matched stars from wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.35 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363_astrometric_residuals.png (954 matched stars from wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.34 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426_astrometric_residuals.png (933 matched stars from wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.51 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427_astrometric_residuals.png (935 matched stars from wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.54 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-05-Q1b1x1_060151_TTUQ1b1x1_731119_dAowQ001/wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits'
Saving fully-calibrated image wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-05-Q1b1x1_060151_TTUQ1b1x1_731119_dAowQ001/wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits'
Preparing the HTML report for the field Aur-05-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:34:36.69 +27:35:32.7: 99.00 +/- 99.00 saturated
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:27:25.46 +25:10:24.0: 9.86 +/- 0.00 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:34:03.30 +26:46:13.7: 99.00 +/- 99.00 saturated
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:31:26.48 +26:17:54.0: 9.47 +/- 0.00 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:30:27.40 +26:01:52.9: 9.28 +/- 0.00 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:32:36.46 +26:17:56.4: 99.00 +/- 99.00 saturated
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:33:38.80 +26:32:07.9: 99.00 +/- 99.00 saturated
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:27:33.09 +24:44:03.7: 99.00 +/- 99.00 saturated
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:33:29.32 +25:28:34.7: 11.23 +/- 0.01 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:32:57.97 +26:00:25.4: 9.57 +/- 0.00 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:34:36.69 +27:35:32.7: 99.00 +/- 99.00 saturated
Forced photometry filter REJECTED candidate at 05:34:36.69 +27:35:32.7: the source is saturated (present but too bright to measure) on at least one reference image -- likely a star-matching failure rather than a new transient
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:31:26.48 +26:17:54.0: 99.00 +/- 99.00 saturated
Forced photometry filter REJECTED candidate at 05:31:26.48 +26:17:54.0: the source is saturated (present but too bright to measure) on at least one reference image -- likely a star-matching failure rather than a new transient
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:32:36.46 +26:17:56.4: 99.00 +/- 99.00 saturated
Forced photometry filter REJECTED candidate at 05:32:36.46 +26:17:56.4: the source is saturated (present but too bright to measure) on at least one reference image -- likely a star-matching failure rather than a new transient
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:30:27.40 +26:01:52.9: 99.00 +/- 99.00 saturated
Forced photometry filter REJECTED candidate at 05:30:27.40 +26:01:52.9: the source is saturated (present but too bright to measure) on at least one reference image -- likely a star-matching failure rather than a new transient
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:34:03.30 +26:46:13.7: 9.28 +/- 0.00 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:27:25.46 +25:10:24.0: 9.87 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 05:34:03.30 +26:46:13.7: the source is saturated (present but too bright to measure) on at least one reference image -- likely a star-matching failure rather than a new transient
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:33:38.80 +26:32:07.9: 99.00 +/- 99.00 saturated
Forced photometry filter REJECTED candidate at 05:33:38.80 +26:32:07.9: the source is saturated (present but too bright to measure) on at least one reference image -- likely a star-matching failure rather than a new transient
Forced photometry reference-image weighted average: 9.86 +/- 0.00
Forced photometry filter REJECTED candidate at 05:27:25.46 +25:10:24.0: ref_mag=9.86 +/- 0.00 new_mean_mag=9.8731 delta=-0.01 (need > 0.90)
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:27:33.09 +24:44:03.7: 99.00 +/- 99.00 saturated
Forced photometry filter REJECTED candidate at 05:27:33.09 +24:44:03.7: the source is saturated (present but too bright to measure) on at least one reference image -- likely a star-matching failure rather than a new transient
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:33:29.32 +25:28:34.7: 11.21 +/- 0.01 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:32:57.97 +26:00:25.4: 9.56 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.22 +/- 0.00
Forced photometry filter KEPT candidate at 05:33:29.32 +25:28:34.7: ref_mag=11.22 +/- 0.00 new_mean_mag=10.0763 delta=1.15 (need > 0.90)
Forced photometry reference-image weighted average: 9.57 +/- 0.00
Forced photometry filter REJECTED candidate at 05:32:57.97 +26:00:25.4: ref_mag=9.57 +/- 0.00 new_mean_mag=10.2273 delta=-0.66 (need > 0.90)
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:33:49.28 +26:38:08.4: 11.04 +/- 0.00 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:31:59.01 +24:59:41.1: 11.03 +/- 0.01 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:33:48.04 +26:29:40.4: 9.51 +/- 0.00 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:32:09.35 +24:59:35.4: 10.95 +/- 0.00 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:34:15.70 +26:48:30.2: 9.75 +/- 0.00 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:29:33.80 +29:20:53.6: 11.35 +/- 0.01 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:26:51.35 +32:03:07.7: 10.29 +/- 0.00 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:33:49.28 +26:38:08.4: 11.05 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.04 +/- 0.00
Forced photometry filter REJECTED candidate at 05:33:49.28 +26:38:08.4: ref_mag=11.04 +/- 0.00 new_mean_mag=10.2836 delta=0.76 (need > 0.90)
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:33:48.04 +26:29:40.4: 9.50 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.50 +/- 0.00
Forced photometry filter REJECTED candidate at 05:33:48.04 +26:29:40.4: ref_mag=9.50 +/- 0.00 new_mean_mag=10.3018 delta=-0.80 (need > 0.90)
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:32:09.35 +24:59:35.4: 10.92 +/- 0.00 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:31:59.01 +24:59:41.1: 11.00 +/- 0.00 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:34:15.70 +26:48:30.2: 9.75 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.93 +/- 0.00
Forced photometry reference-image weighted average: 11.02 +/- 0.00
Forced photometry filter REJECTED candidate at 05:32:09.35 +24:59:35.4: ref_mag=10.93 +/- 0.00 new_mean_mag=10.1858 delta=0.75 (need > 0.90)
Forced photometry reference-image weighted average: 9.75 +/- 0.00
Forced photometry filter REJECTED candidate at 05:31:59.01 +24:59:41.1: ref_mag=11.02 +/- 0.00 new_mean_mag=10.3511 delta=0.67 (need > 0.90)
Forced photometry filter REJECTED candidate at 05:34:15.70 +26:48:30.2: ref_mag=9.75 +/- 0.00 new_mean_mag=10.3808 delta=-0.63 (need > 0.90)
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:30:35.40 +32:47:41.9: 10.63 +/- 0.00 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:29:33.80 +29:20:53.6: 11.34 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.34 +/- 0.00
Forced photometry filter KEPT candidate at 05:29:33.80 +29:20:53.6: ref_mag=11.34 +/- 0.00 new_mean_mag=10.1303 delta=1.21 (need > 0.90)
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:26:51.35 +32:03:07.7: 10.30 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.30 +/- 0.00
Forced photometry filter KEPT candidate at 05:26:51.35 +32:03:07.7: ref_mag=10.30 +/- 0.00 new_mean_mag=9.3786 delta=0.92 (need > 0.90)
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:30:35.40 +32:47:41.9: 10.64 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.63 +/- 0.00
Forced photometry filter KEPT candidate at 05:30:35.40 +32:47:41.9: ref_mag=10.63 +/- 0.00 new_mean_mag=9.4295 delta=1.21 (need > 0.90)
Adding exclusion_list_local.txt__out04242.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05941.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10680.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21197.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 17s
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 21121_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 21121_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 05:29:15.96 +25:09:02.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 21126_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 21126_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 05:31:56.53 +26:41:04.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 21130_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 21130_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 05:33:54.42 +27:09:49.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 21132_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 21132_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 05:32:56.61 +25:53:46.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 21135_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 21135_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 04:38:11.43 +35:13:59.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21143_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 21143_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 05:34:12.32 +26:52:55.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 21145_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 21145_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 05:34:21.55 +27:19:47.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 21149_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 21149_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 05:32:46.54 +26:44:51.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 21152_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 21152_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 05:26:43.67 +25:00:43.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 21155_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 21155_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 05:31:03.44 +26:34:59.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 21156_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 21156_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
Rejecting candidate due to large distance (13.8") between the two second-epoch detections
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Considering the candidate 21159_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 21159_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
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Considering the candidate 21160_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 21160_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
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Considering the candidate 21163_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 21163_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
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Considering the candidate 21166_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 21166_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 05:26:42.43 +25:17:02.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21170_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 21170_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
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Considering the candidate 21176_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 21176_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
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Considering the candidate 21181_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 21181_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 04:38:19.50 +31:18:47.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21186_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 21186_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
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Considering the candidate 21188_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 21188_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
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Considering the candidate 21195_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 21195_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
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Considering the candidate 21197_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
Preparing report for the candidate 21197_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
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Considering the candidate 21204_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 21204_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21213_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 21213_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21214_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 21214_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21215_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 21215_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21220_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 21220_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21223_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 21223_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12406_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 12406_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 04:35:57.48 +28:30:53.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10680_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
Preparing report for the candidate 10680_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06441_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 06441_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 04:51:03.36 +32:09:53.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05941_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
Preparing report for the candidate 05941_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01618_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 01618_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 05:27:07.38 +34:08:57.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04242_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
Preparing report for the candidate 04242_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11604_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 11604_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 05:26:17.31 +28:36:21.0 in the exclusion list exclusion_list_bbsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 21s
Prepared the HTML report for the field Aur-05-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
05:30:35.40 +32:47:41.9
05:26:51.35 +32:03:07.7
05:29:33.80 +29:20:53.6
05:33:29.32 +25:28:34.7
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-05-Q1b1x1_060151_TTUQ1b1x1_731119_dAowQ001/fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-05-Q1b1x1_060151_TTUQ1b1x1_731119_dAowQ001/fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits
SExtractor catalog cache: saved Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat to cache
SExtractor catalog cache: saved Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-05-Q1b1x1_060151_TTUQ1b1x1_731119_dAowQ001/fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-05-Q1b1x1_060151_TTUQ1b1x1_731119_dAowQ001/fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
Creating symlink local_wcs_cache/wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits exists and is non-empty
wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits exists and is non-empty
wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits exists and is non-empty
wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits (1st reference image)
verification OK: wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
Image size: 941.5'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:00:01.017 +29:59:40.48 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits (1st new image)
verification OK: wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits
Image size: 946.9'x627.0' 15.8(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.93"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:00:08.249 +30:02:21.77 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:00:01.017 +29:59:40.48
Second-epoch image center 05:00:08.249 +30:02:21.77
Angular distance between the image centers 0.0518 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits (2nd new image)
verification OK: wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits
Image size: 946.7'x627.0' 15.8(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.93"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:00:05.711 +30:01:43.41 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:00:01.017 +29:59:40.48
Second-epoch image center 05:00:05.711 +30:01:43.41
Angular distance between the image centers 0.0381 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 05:00:08.249 +30:02:21.77
Second-epoch second image center 05:00:05.711 +30:01:43.41
Angular distance between the image centers 0.01405 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/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits &> /tmp/tmp.immL2df88L
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits &> /tmp/tmp.Jlsgs2wYoS
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-05-Q1b1x1_060151_TTUQ1b1x1_731119_dAowQ001/fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits &> /tmp/tmp.qEbPxThmO6
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-05-Q1b1x1_060151_TTUQ1b1x1_731119_dAowQ001/fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-05-Q1b1x1_060151_TTUQ1b1x1_731119_dAowQ001/fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits &> /tmp/tmp.SMQR083LVK
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-05-Q1b1x1_060151_TTUQ1b1x1_731119_dAowQ001/fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.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_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits and wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.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_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits and wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat
Found non-empty wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits and wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat
The reference image (wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits) and catalog (wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat) found
'wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat' -> 'wcsmag.cat'
Read 129003 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 65.5568 to 84.6878 deg, Dec +24.3237 to +35.3004 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 65.5568 to 84.6878 deg, Dec 24.3237 to 35.3004 deg
Loaded 8482 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): 4945 out of 6875 total matches.
Matched with Tycho-2 6875 out of 129003 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.844600
a=0.000000 b=1.000000 c=22.844600
From vast_summary.log: estimated ref. image limiting mag.: -7.27
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.57
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.57
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 129003 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 65.5568 to 84.6878 deg, Dec +24.3237 to +35.3004 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 65.5568 to 84.6878 deg, Dec 24.3237 to 35.3004 deg
Loaded 8482 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): 4945 out of 6875 total matches.
Matched with Tycho-2 6875 out of 129003 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits:
Forced-photometry filter: calibrated wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits -> calib.txt_param_ref_wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits (aperture=4.5)
Read 129055 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 65.5645 to 84.6893 deg, Dec +24.3196 to +35.2959 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 65.5645 to 84.6893 deg, Dec 24.3196 to 35.2959 deg
Loaded 8478 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): 4939 out of 6881 total matches.
Matched with Tycho-2 6881 out of 129055 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits:
Forced-photometry filter: calibrated wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits -> calib.txt_param_ref_wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits (aperture=4.5)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 149 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
1.8 pix Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
1.9 pix Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
2.8 pix fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits
2.8 pix fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits
1.8 pix wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
1.9 pix wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
Limiting magnitude estimates:
15.6 mag. Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
15.6 mag. Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
13.6 mag. fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits
13.6 mag. fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits
All-image limiting magnitude estimate: 13.6 (SNR ) 13.2 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.immL2df88L (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-12_CI_Aur-05-Q1b1x1_060151_TTUQ1b1x1_731119_dAowQ001/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits' -> 'wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
WCS_IMAGE_NAME=wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
WCS-calibrated image found: wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
Checking if the catalog wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat corresponding to the image wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits alredy exist and is non-empty...
Catalog wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat corresponding to the image wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
WCS catalog name: wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.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=36, blended=14027, bad_region=9, passed=128967
Got 128967 stars (including 114713 good ones) from the SExtractor catalog wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat
util/solve_plate_with_UCAC5 got 128967 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
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 951 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 932 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 125973 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 951 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 125971 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 125971 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 951 stars left (next iteration limit 1046)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits N_match=951 sigma_overall_arcsec=0.358 sigma_q1_arcsec=0.383 sigma_q2_arcsec=0.390 sigma_q3_arcsec=0.323 sigma_q4_arcsec=0.320 n_q1=358 n_q2=221 n_q3=209 n_q4=163 worst_quadrant_to_overall_ratio=1.088
The image catalog is written to wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits -region wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.Jlsgs2wYoS (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-12_CI_Aur-05-Q1b1x1_060151_TTUQ1b1x1_731119_dAowQ001/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits' -> 'wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
WCS_IMAGE_NAME=wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
WCS-calibrated image found: wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
Checking if the catalog wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.wcscat corresponding to the image wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits alredy exist and is non-empty...
Catalog wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.wcscat corresponding to the image wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
WCS catalog name: wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.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=35, blended=13827, bad_region=12, passed=129020
Got 129020 stars (including 114961 good ones) from the SExtractor catalog wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.wcscat
util/solve_plate_with_UCAC5 got 129020 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
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 951 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 929 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 126156 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 951 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 126161 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 126159 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 951 stars left (next iteration limit 1046)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits N_match=951 sigma_overall_arcsec=0.357 sigma_q1_arcsec=0.408 sigma_q2_arcsec=0.362 sigma_q3_arcsec=0.327 sigma_q4_arcsec=0.301 n_q1=353 n_q2=224 n_q3=210 n_q4=164 worst_quadrant_to_overall_ratio=1.141
The image catalog is written to wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits -region wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.qEbPxThmO6 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-12_CI_Aur-05-Q1b1x1_060151_TTUQ1b1x1_731119_dAowQ001/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-05-Q1b1x1_060151_TTUQ1b1x1_731119_dAowQ001/fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-05-Q1b1x1_060151_TTUQ1b1x1_731119_dAowQ001/fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-05-Q1b1x1_060151_TTUQ1b1x1_731119_dAowQ001/fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-05-Q1b1x1_060151_TTUQ1b1x1_731119_dAowQ001/fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-05-Q1b1x1_060151_TTUQ1b1x1_731119_dAowQ001/fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-05-Q1b1x1_060151_TTUQ1b1x1_731119_dAowQ001/fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits
WCS_IMAGE_NAME=wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits
WCS-calibrated image found: wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits
Checking if the catalog wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits.wcscat corresponding to the image wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits.wcscat corresponding to the image wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-05-Q1b1x1_060151_TTUQ1b1x1_731119_dAowQ001/fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits
WCS catalog name: wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=1076, bad_region=3, passed=28400
Got 28400 stars (including 27276 good ones) from the SExtractor catalog wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits.wcscat
util/solve_plate_with_UCAC5 got 28400 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 946.9'
Seting catalog search parameters based on the expected field of view 946.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013151 (47.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010521 (37.9 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 629 (Dec 24.1 to 35.5)
Done reading UCAC5 zone files...
Matched 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 896 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 27196 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 629 (Dec 24.1 to 35.5)
Done reading UCAC5 zone files...
Matched 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 27197 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 27197 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Excluding outliers - 927 stars left (next iteration limit 1019)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits N_match=927 sigma_overall_arcsec=0.602 sigma_q1_arcsec=0.587 sigma_q2_arcsec=0.896 sigma_q3_arcsec=0.518 sigma_q4_arcsec=0.638 n_q1=172 n_q2=115 n_q3=298 n_q4=342 worst_quadrant_to_overall_ratio=1.488
The image catalog is written to wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-05-Q1b1x1_060151_TTUQ1b1x1_731119_dAowQ001/fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits -region wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.SMQR083LVK (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-12_CI_Aur-05-Q1b1x1_060151_TTUQ1b1x1_731119_dAowQ001/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-05-Q1b1x1_060151_TTUQ1b1x1_731119_dAowQ001/fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-05-Q1b1x1_060151_TTUQ1b1x1_731119_dAowQ001/fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-05-Q1b1x1_060151_TTUQ1b1x1_731119_dAowQ001/fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-05-Q1b1x1_060151_TTUQ1b1x1_731119_dAowQ001/fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-05-Q1b1x1_060151_TTUQ1b1x1_731119_dAowQ001/fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-05-Q1b1x1_060151_TTUQ1b1x1_731119_dAowQ001/fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits
WCS_IMAGE_NAME=wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits
WCS-calibrated image found: wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits
Checking if the catalog wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits.wcscat corresponding to the image wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits.wcscat corresponding to the image wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-05-Q1b1x1_060151_TTUQ1b1x1_731119_dAowQ001/fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits
WCS catalog name: wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=1152, bad_region=3, passed=28723
Got 28723 stars (including 27524 good ones) from the SExtractor catalog wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits.wcscat
util/solve_plate_with_UCAC5 got 28723 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 946.7'
Seting catalog search parameters based on the expected field of view 946.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013149 (47.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010519 (37.9 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 629 (Dec 24.1 to 35.4)
Done reading UCAC5 zone files...
Matched 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 899 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 27443 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
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 629 (Dec 24.1 to 35.4)
Done reading UCAC5 zone files...
Matched 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 27441 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 27441 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Excluding outliers - 929 stars left (next iteration limit 1021)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits N_match=929 sigma_overall_arcsec=0.620 sigma_q1_arcsec=0.663 sigma_q2_arcsec=0.843 sigma_q3_arcsec=0.511 sigma_q4_arcsec=0.640 n_q1=170 n_q2=117 n_q3=302 n_q4=340 worst_quadrant_to_overall_ratio=1.360
The image catalog is written to wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-05-Q1b1x1_060151_TTUQ1b1x1_731119_dAowQ001/fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits -region wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-05-Q1b1x1_060151_TTUQ1b1x1_731119_dAowQ001/wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-11-12_20.00sec_0.00C_LIGHTs_0426.fits
Saving fully-calibrated image wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-05-Q1b1x1_060151_TTUQ1b1x1_731119_dAowQ001/wcs_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427.fits
Preparing the HTML report for the field Aur-05-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:16:03.61 +33:04:43.5: 12.58 +/- 0.01 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:32:57.97 +26:00:25.3: 9.57 +/- 0.00 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:32:36.46 +26:17:56.4: 99.00 +/- 99.00 saturated
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:33:38.79 +26:32:07.9: 99.00 +/- 99.00 saturated
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:33:48.03 +26:29:40.4: 9.52 +/- 0.00 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 04:34:18.76 +30:23:06.6: 16.06 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:30:35.35 +24:49:10.7: 11.14 +/- 0.00 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:34:15.67 +26:48:30.5: 9.74 +/- 0.00 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:33:24.53 +26:32:57.0: 10.41 +/- 0.00 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:16:03.61 +33:04:43.5: 12.56 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.57 +/- 0.01
Forced photometry filter REJECTED candidate at 05:16:03.61 +33:04:43.5: ref_mag=12.57 +/- 0.01 new_mean_mag=12.4311 delta=0.14 (need > 0.90)
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:32:57.97 +26:00:25.3: 9.55 +/- 0.00 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:32:36.46 +26:17:56.4: 99.00 +/- 99.00 saturated
Forced photometry filter REJECTED candidate at 05:32:36.46 +26:17:56.4: the source is saturated (present but too bright to measure) on at least one reference image -- likely a star-matching failure rather than a new transient
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:33:38.79 +26:32:07.9: 99.00 +/- 99.00 saturated
Forced photometry filter REJECTED candidate at 05:33:38.79 +26:32:07.9: the source is saturated (present but too bright to measure) on at least one reference image -- likely a star-matching failure rather than a new transient
Forced photometry reference-image weighted average: 9.56 +/- 0.00
Forced photometry filter REJECTED candidate at 05:32:57.97 +26:00:25.3: ref_mag=9.56 +/- 0.00 new_mean_mag=10.3065 delta=-0.75 (need > 0.90)
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:33:48.03 +26:29:40.4: 9.51 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.51 +/- 0.00
Forced photometry filter REJECTED candidate at 05:33:48.03 +26:29:40.4: ref_mag=9.51 +/- 0.00 new_mean_mag=10.4062 delta=-0.89 (need > 0.90)
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:34:15.67 +26:48:30.5: 9.73 +/- 0.00 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:30:35.35 +24:49:10.7: 11.18 +/- 0.00 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 04:34:18.76 +30:23:06.6: 16.08 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 11.16 +/- 0.00
Forced photometry reference-image weighted average: 9.74 +/- 0.00
Forced photometry filter REJECTED candidate at 05:30:35.35 +24:49:10.7: ref_mag=11.16 +/- 0.00 new_mean_mag=10.6143 delta=0.55 (need > 0.90)
Forced photometry filter REJECTED candidate at 05:34:15.67 +26:48:30.5: ref_mag=9.74 +/- 0.00 new_mean_mag=10.4937 delta=-0.76 (need > 0.90)
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:33:24.53 +26:32:57.0: 10.40 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.40 +/- 0.00
Forced photometry filter REJECTED candidate at 05:33:24.53 +26:32:57.0: ref_mag=10.40 +/- 0.00 new_mean_mag=10.7893 delta=-0.38 (need > 0.90)
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:32:32.28 +26:08:15.6: 10.09 +/- 0.00 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:32:21.08 +25:21:16.9: 12.06 +/- 0.01 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:33:16.58 +26:31:11.7: 10.52 +/- 0.00 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:32:32.28 +26:08:15.6: 10.11 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.10 +/- 0.00
Forced photometry filter REJECTED candidate at 05:32:32.28 +26:08:15.6: ref_mag=10.10 +/- 0.00 new_mean_mag=10.7987 delta=-0.70 (need > 0.90)
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:33:49.48 +26:23:30.7: 9.95 +/- 0.00 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:30:17.02 +25:08:24.5: 11.44 +/- 0.01 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:28:12.80 +24:33:55.8: 11.70 +/- 0.01 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:31:43.65 +25:46:13.7: 10.98 +/- 0.00 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:31:21.38 +25:18:46.2: 11.38 +/- 0.01 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:33:12.44 +26:31:47.3: 10.25 +/- 0.00 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:33:16.58 +26:31:11.7: 10.55 +/- 0.00 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:32:21.08 +25:21:16.9: 12.12 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.53 +/- 0.00
Forced photometry reference-image weighted average: 12.09 +/- 0.01
Forced photometry filter REJECTED candidate at 05:33:16.58 +26:31:11.7: ref_mag=10.53 +/- 0.00 new_mean_mag=10.9127 delta=-0.38 (need > 0.90)
Forced photometry filter KEPT candidate at 05:32:21.08 +25:21:16.9: ref_mag=12.09 +/- 0.01 new_mean_mag=10.9653 delta=1.12 (need > 0.90)
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:33:49.48 +26:23:30.7: 9.96 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.95 +/- 0.00
Forced photometry filter REJECTED candidate at 05:33:49.48 +26:23:30.7: ref_mag=9.95 +/- 0.00 new_mean_mag=10.9407 delta=-0.99 (need > 0.90)
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:30:17.02 +25:08:24.5: 11.46 +/- 0.01 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:31:43.65 +25:46:13.7: 10.98 +/- 0.00 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:28:12.80 +24:33:55.8: 11.71 +/- 0.01 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:31:21.38 +25:18:46.2: 11.38 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.98 +/- 0.00
Forced photometry reference-image weighted average: 11.45 +/- 0.00
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:33:12.44 +26:31:47.3: 10.27 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.71 +/- 0.01
Forced photometry filter REJECTED candidate at 05:31:43.65 +25:46:13.7: ref_mag=10.98 +/- 0.00 new_mean_mag=11.0368 delta=-0.06 (need > 0.90)
Forced photometry filter REJECTED candidate at 05:30:17.02 +25:08:24.5: ref_mag=11.45 +/- 0.00 new_mean_mag=11.0933 delta=0.36 (need > 0.90)
Forced photometry reference-image weighted average: 11.38 +/- 0.00
Forced photometry filter REJECTED candidate at 05:28:12.80 +24:33:55.8: ref_mag=11.71 +/- 0.01 new_mean_mag=11.0837 delta=0.62 (need > 0.90)
Forced photometry filter REJECTED candidate at 05:31:21.38 +25:18:46.2: ref_mag=11.38 +/- 0.00 new_mean_mag=11.1247 delta=0.26 (need > 0.90)
Forced photometry reference-image weighted average: 10.26 +/- 0.00
Forced photometry filter REJECTED candidate at 05:33:12.44 +26:31:47.3: ref_mag=10.26 +/- 0.00 new_mean_mag=11.1080 delta=-0.85 (need > 0.90)
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:32:43.71 +25:46:55.9: 11.51 +/- 0.01 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:28:50.24 +33:29:34.2: 15.74 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:32:43.71 +25:46:55.9: 11.52 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.52 +/- 0.00
Forced photometry filter REJECTED candidate at 05:32:43.71 +25:46:55.9: ref_mag=11.52 +/- 0.00 new_mean_mag=11.0699 delta=0.45 (need > 0.90)
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:33:05.21 +25:07:43.7: 13.39 +/- 0.04 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:28:50.24 +33:29:34.2: 15.81 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:33:32.78 +25:43:15.4: 12.64 +/- 0.02 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:28:35.69 +24:38:11.1: 10.96 +/- 0.00 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:29:37.37 +25:19:52.0: 10.99 +/- 0.00 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:33:05.21 +25:07:43.7: 13.37 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.03
Forced photometry filter KEPT candidate at 05:33:05.21 +25:07:43.7: ref_mag=13.38 +/- 0.03 new_mean_mag=11.2622 delta=2.12 (need > 0.90)
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 04:40:28.16 +30:16:48.8: 16.07 +/- 0.31 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:33:32.78 +25:43:15.4: 12.62 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.01
Forced photometry filter KEPT candidate at 05:33:32.78 +25:43:15.4: ref_mag=12.63 +/- 0.01 new_mean_mag=11.4167 delta=1.21 (need > 0.90)
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:28:35.69 +24:38:11.1: 10.98 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.97 +/- 0.00
Forced photometry filter REJECTED candidate at 05:28:35.69 +24:38:11.1: ref_mag=10.97 +/- 0.00 new_mean_mag=11.3340 delta=-0.36 (need > 0.90)
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:29:37.37 +25:19:52.0: 10.99 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.99 +/- 0.00
Forced photometry filter REJECTED candidate at 05:29:37.37 +25:19:52.0: ref_mag=10.99 +/- 0.00 new_mean_mag=11.4929 delta=-0.50 (need > 0.90)
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:34:16.45 +26:50:48.9: 11.36 +/- 0.01 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:30:40.76 +25:01:44.1: 12.49 +/- 0.02 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 04:40:28.16 +30:16:48.8: 16.25 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 16.07 +/- 0.31
Forced photometry filter KEPT candidate at 04:40:28.16 +30:16:48.8: ref_mag=16.07 +/- 0.31 new_mean_mag=12.4607 delta=3.61 (need > 0.90)
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:34:16.45 +26:50:48.9: 11.35 +/- 0.01 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:30:40.76 +25:01:44.1: 12.50 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.35 +/- 0.00
Forced photometry filter REJECTED candidate at 05:34:16.45 +26:50:48.9: ref_mag=11.35 +/- 0.00 new_mean_mag=11.6366 delta=-0.28 (need > 0.90)
Forced photometry reference-image weighted average: 12.50 +/- 0.01
Forced photometry filter REJECTED candidate at 05:30:40.76 +25:01:44.1: ref_mag=12.50 +/- 0.01 new_mean_mag=11.6152 delta=0.88 (need > 0.90)
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:30:40.50 +24:58:35.0: 12.28 +/- 0.01 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:27:56.40 +24:26:32.4: 99.00 +/- 99.00 edge
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:30:40.50 +24:58:35.0: 12.30 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.29 +/- 0.01
Forced photometry filter REJECTED candidate at 05:30:40.50 +24:58:35.0: ref_mag=12.29 +/- 0.01 new_mean_mag=11.7494 delta=0.54 (need > 0.90)
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:27:56.40 +24:26:32.4: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 05:27:56.40 +24:26:32.4: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:19:44.27 +26:10:31.3: 15.53 +/- 0.20 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:31:03.09 +24:58:11.2: 12.97 +/- 0.02 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:31:00.66 +25:12:34.0: 12.18 +/- 0.01 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:19:44.27 +26:10:31.3: 15.43 +/- 0.19 detection
Forced photometry reference-image weighted average: 15.48 +/- 0.14
Forced photometry filter KEPT candidate at 05:19:44.27 +26:10:31.3: ref_mag=15.48 +/- 0.14 new_mean_mag=12.0710 delta=3.41 (need > 0.90)
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:31:00.66 +25:12:34.0: 12.17 +/- 0.01 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:31:03.09 +24:58:11.2: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.17 +/- 0.01
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 04:41:59.18 +35:15:30.1: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 05:31:00.66 +25:12:34.0: ref_mag=12.17 +/- 0.01 new_mean_mag=11.9039 delta=0.27 (need > 0.90)
Forced photometry reference-image weighted average: 12.94 +/- 0.02
Forced photometry filter KEPT candidate at 05:31:03.09 +24:58:11.2: ref_mag=12.94 +/- 0.02 new_mean_mag=11.9142 delta=1.03 (need > 0.90)
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:33:36.58 +26:34:24.3: 10.97 +/- 0.00 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 04:41:59.18 +35:15:30.1: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 04:41:59.18 +35:15:30.1: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:30:35.26 +25:13:36.6: 12.37 +/- 0.01 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:33:36.58 +26:34:24.3: 10.96 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.97 +/- 0.00
Forced photometry filter REJECTED candidate at 05:33:36.58 +26:34:24.3: ref_mag=10.97 +/- 0.00 new_mean_mag=11.8478 delta=-0.88 (need > 0.90)
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:29:44.11 +24:25:37.9: 99.00 +/- 99.00 edge
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:30:35.26 +25:13:36.6: 12.40 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.38 +/- 0.01
Forced photometry filter REJECTED candidate at 05:30:35.26 +25:13:36.6: ref_mag=12.38 +/- 0.01 new_mean_mag=12.0384 delta=0.34 (need > 0.90)
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:29:44.11 +24:25:37.9: 13.20 +/- 0.03 detection
Forced photometry filter REJECTED candidate at 05:29:44.11 +24:25:37.9: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 04:45:17.75 +31:12:11.8: 13.98 +/- 0.05 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:20:40.99 +32:46:02.3: 13.17 +/- 0.03 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 04:45:17.75 +31:12:11.8: 13.97 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.97 +/- 0.03
Forced photometry filter KEPT candidate at 04:45:17.75 +31:12:11.8: ref_mag=13.97 +/- 0.03 new_mean_mag=12.9744 delta=1.00 (need > 0.90)
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:20:40.99 +32:46:02.3: 13.19 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.02
Forced photometry filter KEPT candidate at 05:20:40.99 +32:46:02.3: ref_mag=13.18 +/- 0.02 new_mean_mag=12.1743 delta=1.01 (need > 0.90)
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 04:52:40.42 +29:13:59.8: 13.38 +/- 0.03 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 04:52:40.42 +29:13:59.8: 13.36 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.02
Forced photometry filter KEPT candidate at 04:52:40.42 +29:13:59.8: ref_mag=13.37 +/- 0.02 new_mean_mag=12.4037 delta=0.97 (need > 0.90)
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:16:23.38 +31:33:47.1: 13.97 +/- 0.05 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:16:23.38 +31:33:47.1: 13.86 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.91 +/- 0.03
Forced photometry filter KEPT candidate at 05:16:23.38 +31:33:47.1: ref_mag=13.91 +/- 0.03 new_mean_mag=12.8316 delta=1.08 (need > 0.90)
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:01:05.18 +32:51:54.4: 13.06 +/- 0.02 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 04:59:57.74 +27:26:58.9: 13.64 +/- 0.03 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:01:05.18 +32:51:54.4: 13.10 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.01
Forced photometry filter KEPT candidate at 05:01:05.18 +32:51:54.4: ref_mag=13.08 +/- 0.01 new_mean_mag=12.1550 delta=0.93 (need > 0.90)
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 04:59:57.74 +27:26:58.9: 13.69 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.02
Forced photometry filter KEPT candidate at 04:59:57.74 +27:26:58.9: ref_mag=13.67 +/- 0.02 new_mean_mag=12.7180 delta=0.95 (need > 0.90)
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:20:58.54 +25:08:44.2: 12.40 +/- 0.01 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:20:58.54 +25:08:44.2: 12.45 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.42 +/- 0.01
Forced photometry filter KEPT candidate at 05:20:58.54 +25:08:44.2: ref_mag=12.42 +/- 0.01 new_mean_mag=11.4137 delta=1.01 (need > 0.90)
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:12:02.91 +32:26:56.3: 13.86 +/- 0.04 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:12:02.91 +32:26:56.3: 13.87 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.86 +/- 0.03
Forced photometry filter KEPT candidate at 05:12:02.91 +32:26:56.3: ref_mag=13.86 +/- 0.03 new_mean_mag=12.8345 delta=1.03 (need > 0.90)
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:05:08.99 +25:22:10.4: 13.64 +/- 0.04 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:05:08.99 +25:22:10.4: 13.59 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.02
Forced photometry filter KEPT candidate at 05:05:08.99 +25:22:10.4: ref_mag=13.61 +/- 0.02 new_mean_mag=12.4092 delta=1.20 (need > 0.90)
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 04:45:50.66 +28:10:28.4: 13.61 +/- 0.03 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 04:58:45.63 +32:09:05.0: 13.86 +/- 0.04 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 04:45:50.66 +28:10:28.4: 13.64 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.02
Forced photometry filter KEPT candidate at 04:45:50.66 +28:10:28.4: ref_mag=13.62 +/- 0.02 new_mean_mag=12.5204 delta=1.10 (need > 0.90)
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 04:58:45.63 +32:09:05.0: 13.96 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.91 +/- 0.03
Forced photometry filter KEPT candidate at 04:58:45.63 +32:09:05.0: ref_mag=13.91 +/- 0.03 new_mean_mag=12.9168 delta=0.99 (need > 0.90)
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:08:43.29 +26:03:10.8: 12.29 +/- 0.01 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:08:43.29 +26:03:10.8: 12.31 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.30 +/- 0.01
Forced photometry filter KEPT candidate at 05:08:43.29 +26:03:10.8: ref_mag=12.30 +/- 0.01 new_mean_mag=11.3571 delta=0.95 (need > 0.90)
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:07:35.82 +29:00:15.8: 12.81 +/- 0.02 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:06:29.74 +29:26:30.7: 13.03 +/- 0.02 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:07:35.82 +29:00:15.8: 12.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.01
Forced photometry filter KEPT candidate at 05:07:35.82 +29:00:15.8: ref_mag=12.81 +/- 0.01 new_mean_mag=11.5161 delta=1.29 (need > 0.90)
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:06:29.74 +29:26:30.7: 13.05 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.01
Forced photometry filter KEPT candidate at 05:06:29.74 +29:26:30.7: ref_mag=13.04 +/- 0.01 new_mean_mag=12.0009 delta=1.04 (need > 0.90)
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 04:53:30.35 +31:26:31.6: 12.26 +/- 0.01 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 04:53:30.35 +31:26:31.6: 12.26 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.26 +/- 0.01
Forced photometry filter KEPT candidate at 04:53:30.35 +31:26:31.6: ref_mag=12.26 +/- 0.01 new_mean_mag=11.2475 delta=1.01 (need > 0.90)
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:05:51.08 +26:46:29.3: 13.81 +/- 0.04 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:05:51.08 +26:46:29.3: 13.72 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.76 +/- 0.03
Forced photometry filter KEPT candidate at 05:05:51.08 +26:46:29.3: ref_mag=13.76 +/- 0.03 new_mean_mag=12.6591 delta=1.10 (need > 0.90)
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:02:50.79 +28:43:15.6: 12.78 +/- 0.01 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:02:50.79 +28:43:15.6: 12.72 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.75 +/- 0.01
Forced photometry filter KEPT candidate at 05:02:50.79 +28:43:15.6: ref_mag=12.75 +/- 0.01 new_mean_mag=11.7682 delta=0.98 (need > 0.90)
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:06:18.62 +28:34:06.1: 12.20 +/- 0.01 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:06:18.62 +28:34:06.1: 12.17 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.19 +/- 0.01
Forced photometry filter KEPT candidate at 05:06:18.62 +28:34:06.1: ref_mag=12.19 +/- 0.01 new_mean_mag=11.2598 delta=0.93 (need > 0.90)
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:01:21.17 +30:48:07.8: 13.79 +/- 0.04 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:02:01.97 +31:29:34.1: 13.79 +/- 0.04 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 04:59:02.06 +31:50:19.3: 14.93 +/- 0.11 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:01:21.17 +30:48:07.8: 13.82 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.03
Forced photometry filter KEPT candidate at 05:01:21.17 +30:48:07.8: ref_mag=13.81 +/- 0.03 new_mean_mag=12.6131 delta=1.19 (need > 0.90)
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:02:01.97 +31:29:34.1: 13.66 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.03
Forced photometry filter REJECTED candidate at 05:02:01.97 +31:29:34.1: ref_mag=13.71 +/- 0.03 new_mean_mag=12.8903 delta=0.82 (need > 0.90)
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 04:59:02.06 +31:50:19.3: 15.18 +/- 0.14 detection
Forced photometry reference-image weighted average: 15.02 +/- 0.09
Forced photometry filter KEPT candidate at 04:59:02.06 +31:50:19.3: ref_mag=15.02 +/- 0.09 new_mean_mag=13.2627 delta=1.76 (need > 0.90)
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:18:31.28 +27:01:53.9: 13.53 +/- 0.03 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:18:31.28 +27:01:53.9: 13.54 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.54 +/- 0.02
Forced photometry filter KEPT candidate at 05:18:31.28 +27:01:53.9: ref_mag=13.54 +/- 0.02 new_mean_mag=12.4822 delta=1.05 (need > 0.90)
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 04:38:07.76 +29:58:31.9: 12.93 +/- 0.02 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:06:14.13 +32:02:13.4: 13.70 +/- 0.03 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 04:38:07.76 +29:58:31.9: 12.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.01
Forced photometry filter KEPT candidate at 04:38:07.76 +29:58:31.9: ref_mag=12.93 +/- 0.01 new_mean_mag=11.9795 delta=0.95 (need > 0.90)
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:06:14.13 +32:02:13.4: 13.73 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.72 +/- 0.02
Forced photometry filter KEPT candidate at 05:06:14.13 +32:02:13.4: ref_mag=13.72 +/- 0.02 new_mean_mag=12.6659 delta=1.05 (need > 0.90)
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:18:54.39 +25:01:24.8: 12.65 +/- 0.02 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:22:54.04 +27:26:39.4: 13.32 +/- 0.03 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:18:54.39 +25:01:24.8: 12.69 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.01
Forced photometry filter KEPT candidate at 05:18:54.39 +25:01:24.8: ref_mag=12.67 +/- 0.01 new_mean_mag=11.6294 delta=1.04 (need > 0.90)
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:22:54.04 +27:26:39.4: 13.32 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.02
Forced photometry filter KEPT candidate at 05:22:54.04 +27:26:39.4: ref_mag=13.32 +/- 0.02 new_mean_mag=12.1705 delta=1.15 (need > 0.90)
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 04:51:12.37 +25:58:31.7: 14.51 +/- 0.08 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:01:11.29 +32:26:10.7: 14.31 +/- 0.06 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 04:51:12.37 +25:58:31.7: 14.34 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.41 +/- 0.05
Forced photometry filter KEPT candidate at 04:51:12.37 +25:58:31.7: ref_mag=14.41 +/- 0.05 new_mean_mag=12.8540 delta=1.56 (need > 0.90)
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:01:11.29 +32:26:10.7: 14.36 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.33 +/- 0.04
Forced photometry filter KEPT candidate at 05:01:11.29 +32:26:10.7: ref_mag=14.33 +/- 0.04 new_mean_mag=12.9182 delta=1.41 (need > 0.90)
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:25:49.97 +30:05:45.3: 12.59 +/- 0.02 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:25:49.97 +30:05:45.3: 12.65 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.01
Forced photometry filter KEPT candidate at 05:25:49.97 +30:05:45.3: ref_mag=12.62 +/- 0.01 new_mean_mag=11.5391 delta=1.08 (need > 0.90)
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:02:27.13 +32:51:56.9: 13.24 +/- 0.02 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:07:49.51 +30:24:04.3: 12.52 +/- 0.01 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:02:27.13 +32:51:56.9: 13.27 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.25 +/- 0.02
Forced photometry filter KEPT candidate at 05:02:27.13 +32:51:56.9: ref_mag=13.25 +/- 0.02 new_mean_mag=12.2609 delta=0.99 (need > 0.90)
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:06:16.52 +27:22:15.4: 12.52 +/- 0.01 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:05:26.34 +31:29:49.7: 14.31 +/- 0.06 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:07:49.51 +30:24:04.3: 12.50 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.51 +/- 0.01
Forced photometry filter KEPT candidate at 05:07:49.51 +30:24:04.3: ref_mag=12.51 +/- 0.01 new_mean_mag=11.5491 delta=0.96 (need > 0.90)
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:06:16.52 +27:22:15.4: 12.52 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.52 +/- 0.01
Forced photometry filter KEPT candidate at 05:06:16.52 +27:22:15.4: ref_mag=12.52 +/- 0.01 new_mean_mag=11.3512 delta=1.17 (need > 0.90)
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:05:26.34 +31:29:49.7: 14.25 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.28 +/- 0.04
Forced photometry filter KEPT candidate at 05:05:26.34 +31:29:49.7: ref_mag=14.28 +/- 0.04 new_mean_mag=13.1631 delta=1.12 (need > 0.90)
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:33:23.04 +29:29:45.3: 12.46 +/- 0.01 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:33:23.04 +29:29:45.3: 12.50 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.48 +/- 0.01
Forced photometry filter KEPT candidate at 05:33:23.04 +29:29:45.3: ref_mag=12.48 +/- 0.01 new_mean_mag=11.4037 delta=1.08 (need > 0.90)
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:13:59.20 +31:03:18.6: 12.41 +/- 0.01 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:13:59.20 +31:03:18.6: 12.44 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.42 +/- 0.01
Forced photometry filter KEPT candidate at 05:13:59.20 +31:03:18.6: ref_mag=12.42 +/- 0.01 new_mean_mag=11.3245 delta=1.10 (need > 0.90)
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:00:23.24 +30:32:35.9: 13.92 +/- 0.04 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:00:23.24 +30:32:35.9: 13.91 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.92 +/- 0.03
Forced photometry filter REJECTED candidate at 05:00:23.24 +30:32:35.9: ref_mag=13.92 +/- 0.03 new_mean_mag=13.0440 delta=0.87 (need > 0.90)
Adding exclusion_list_gaiadr2.txt__out151530.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out101102.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103810.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104277.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out110472.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out113106.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out113941.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out117170.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out121425.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out123731.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out128910.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151359.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151399.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151430.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151463.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151499.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151691.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151726.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33363.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34872.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34959.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39926.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41372.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out45640.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46603.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50196.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51922.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54309.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55351.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out58936.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out59132.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out64643.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out70065.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out70734.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out76838.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77691.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out84209.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out88207.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out89704.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95321.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out96408.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out96888.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 22s
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: 22s
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Considering the candidate 151199_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 151199_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 04:54:31.25 +33:17:45.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 151203_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 151203_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
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Considering the candidate 151205_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 151205_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 04:33:04.51 +29:46:45.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 151234_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 151234_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 05:32:56.71 +25:53:45.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 151237_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 151237_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 04:38:11.40 +35:13:59.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 151267_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 151267_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
Rejecting candidate due to large distance (14.0") between the two second-epoch detections
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Considering the candidate 151274_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 151274_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
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Considering the candidate 151296_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 151296_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
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Considering the candidate 151303_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 151303_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 05:33:29.33 +25:28:34.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 151317_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 151317_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
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Considering the candidate 151328_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 151328_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
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Considering the candidate 151336_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 151336_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
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Considering the candidate 151352_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 151352_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
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Considering the candidate 151359_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
Preparing report for the candidate 151359_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
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Considering the candidate 151363_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 151363_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 151364_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 151364_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
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Considering the candidate 151373_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 151373_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
Rejecting candidate due to large distance (39.3") between the two second-epoch detections
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Considering the candidate 151374_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 151374_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
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Considering the candidate 151378_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 151378_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 04:56:57.83 +33:05:59.5 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 151385_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 151385_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
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Considering the candidate 151399_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
Preparing report for the candidate 151399_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
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Considering the candidate 151405_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 151405_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 04:41:14.20 +28:37:40.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 151413_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 151413_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
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Considering the candidate 151414_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 151414_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
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Considering the candidate 151415_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 151415_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
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Considering the candidate 151419_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 151419_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
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Considering the candidate 151421_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 151421_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
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Considering the candidate 151423_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 151423_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
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Considering the candidate 151428_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 151428_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
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Considering the candidate 151430_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
Preparing report for the candidate 151430_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
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Considering the candidate 151439_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 151439_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 05:18:18.04 +33:47:33.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 151463_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
Preparing report for the candidate 151463_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
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Considering the candidate 151466_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 151466_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 05:27:41.45 +34:26:43.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 151480_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 151480_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 04:56:56.89 +33:06:50.5 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 151486_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 151486_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 05:06:25.48 +34:49:30.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 151495_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 151495_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 04:24:35.98 +34:06:48.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 151499_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
Preparing report for the candidate 151499_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
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Considering the candidate 151512_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 151512_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
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Considering the candidate 151517_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 151517_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 05:36:07.76 +34:09:24.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 151519_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 151519_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 05:36:28.04 +34:07:48.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 151528_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 151528_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
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Considering the candidate 151529_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 151529_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 05:36:28.31 +34:07:23.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 151530_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 151530_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 04:40:28.16 +30:16:48.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 1.977 159334151287938048 070.11678363421 +30.28049837297 11.8664 10.0854 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.977#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151543_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 151543_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 151549_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 151549_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
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Considering the candidate 151551_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 151551_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
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Considering the candidate 151557_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 151557_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 04:32:24.98 +30:30:52.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 151574_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 151574_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 05:15:29.76 +32:42:37.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 151575_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 151575_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 05:14:46.54 +31:23:49.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 151581_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 151581_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 04:38:26.86 +26:55:00.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 151588_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 151588_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
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Considering the candidate 151590_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 151590_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
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Considering the candidate 151596_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 151596_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 04:30:05.79 +32:29:46.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 151599_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 151599_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 04:24:35.40 +34:07:13.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 151636_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 151636_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 04:57:04.31 +33:12:25.3 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 151646_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 151646_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 05:22:00.58 +32:53:51.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 151669_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 151669_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 04:59:17.78 +32:33:35.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 151691_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
Preparing report for the candidate 151691_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
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Considering the candidate 151726_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
Preparing report for the candidate 151726_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
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Considering the candidate 151727_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 151727_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
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Considering the candidate 151730_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 151730_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 04:51:21.96 +28:31:15.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 151732_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 151732_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 05:26:40.68 +34:23:16.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 151754_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 151754_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
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Considering the candidate 151755_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 151755_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 05:10:01.86 +26:45:55.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 151757_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 151757_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
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Considering the candidate 151773_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 151773_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
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Considering the candidate 151844_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 151844_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
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Considering the candidate 151887_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 151887_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 04:26:35.64 +31:24:00.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 121345_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 121345_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 05:03:15.44 +28:42:52.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57253_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 57253_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 04:38:19.52 +31:18:47.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 59132_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
Preparing report for the candidate 59132_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
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Considering the candidate 33363_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
Preparing report for the candidate 33363_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
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Considering the candidate 108616_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 108616_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 05:06:08.24 +27:03:20.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 88207_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
Preparing report for the candidate 88207_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
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Considering the candidate 51922_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
Preparing report for the candidate 51922_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
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Considering the candidate 144413_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 144413_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 05:10:32.25 +32:10:42.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 34959_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
Preparing report for the candidate 34959_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
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Considering the candidate 113941_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
Preparing report for the candidate 113941_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
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Considering the candidate 96408_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
Preparing report for the candidate 96408_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
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Considering the candidate 80620_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 80620_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 04:32:50.32 +29:42:38.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 39926_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
Preparing report for the candidate 39926_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
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Considering the candidate 16878_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 16878_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 05:10:41.89 +33:57:12.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 96888_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
Preparing report for the candidate 96888_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
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Considering the candidate 80722_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 80722_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 05:29:33.80 +29:20:53.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 17435_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 17435_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 04:59:52.38 +33:59:04.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 123731_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
Preparing report for the candidate 123731_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
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Considering the candidate 45640_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
Preparing report for the candidate 45640_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
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Considering the candidate 106934_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 106934_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 04:55:57.18 +26:05:43.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103810_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
Preparing report for the candidate 103810_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
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Considering the candidate 128113_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 128113_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 04:35:57.48 +28:30:53.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 89704_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
Preparing report for the candidate 89704_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
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Considering the candidate 84209_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
Preparing report for the candidate 84209_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
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Considering the candidate 55351_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
Preparing report for the candidate 55351_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
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Considering the candidate 107910_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 107910_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 05:09:07.38 +26:08:20.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 104277_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
Preparing report for the candidate 104277_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
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Considering the candidate 121425_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
Preparing report for the candidate 121425_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
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Considering the candidate 44278_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 44278_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 04:51:03.38 +32:09:53.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 128910_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
Preparing report for the candidate 128910_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
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Considering the candidate 14221_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 14221_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 04:36:04.35 +34:10:42.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 97196_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 97196_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 05:04:49.33 +25:24:54.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 64643_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
Preparing report for the candidate 64643_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
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Considering the candidate 54729_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 54729_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
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Considering the candidate 50196_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
Preparing report for the candidate 50196_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
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Considering the candidate 110472_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
Preparing report for the candidate 110472_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
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Considering the candidate 29397_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 29397_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 05:30:35.38 +32:47:41.4 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 103574_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 103574_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 04:46:44.44 +26:23:06.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105568_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 105568_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 05:15:47.34 +26:45:14.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 76838_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
Preparing report for the candidate 76838_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
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Considering the candidate 46603_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
Preparing report for the candidate 46603_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
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Considering the candidate 33728_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 33728_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 04:39:12.09 +32:54:35.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 95321_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
Preparing report for the candidate 95321_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
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Considering the candidate 117170_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
Preparing report for the candidate 117170_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
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Considering the candidate 08465_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 08465_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 05:00:49.68 +34:37:53.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101102_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
Preparing report for the candidate 101102_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
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Considering the candidate 41372_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
Preparing report for the candidate 41372_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
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Considering the candidate 40884_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 40884_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 05:26:51.34 +32:03:07.7 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 70734_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
Preparing report for the candidate 70734_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
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Considering the candidate 09926_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 09926_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 05:27:07.37 +34:08:57.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 01960_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 01960_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 04:59:47.43 +35:03:00.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57431_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 57431_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 04:54:58.11 +31:19:12.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 34872_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
Preparing report for the candidate 34872_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
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Considering the candidate 70065_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
Preparing report for the candidate 70065_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
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Considering the candidate 113106_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
Preparing report for the candidate 113106_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
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Considering the candidate 139674_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 139674_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 05:24:55.52 +30:10:39.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54309_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
Preparing report for the candidate 54309_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
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Considering the candidate 11714_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 11714_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 05:28:37.23 +34:02:26.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 139641_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 139641_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 05:26:52.90 +30:33:46.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 77691_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
Preparing report for the candidate 77691_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
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Considering the candidate 20855_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 20855_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 05:23:15.72 +33:32:07.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33758_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 33758_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 05:28:52.82 +32:28:37.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 66692_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 66692_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 05:04:14.46 +30:29:38.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 75122_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 75122_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 05:11:38.21 +29:54:11.3 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 122846_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 122846_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 05:09:45.16 +28:01:49.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 119884_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 119884_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 04:52:47.34 +27:53:50.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25109_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 25109_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 04:56:59.71 +33:09:52.5 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72001_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 72001_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 05:27:10.28 +29:55:15.0 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58936_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
Preparing report for the candidate 58936_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33443_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 33443_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 05:15:24.11 +32:41:12.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 78812_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 78812_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 05:21:12.57 +29:34:11.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 28396_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 28396_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 05:33:43.15 +32:44:56.0 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21034_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 21034_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 05:18:10.52 +33:22:10.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 94158_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 94158_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 04:58:09.47 +25:03:00.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68788_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 68788_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 88342_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 88342_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 05:26:17.31 +28:36:20.9 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04550_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 04550_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 05:27:38.77 +34:28:30.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12946_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 12946_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 05:20:00.84 +33:57:27.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 37087_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 37087_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 05:32:43.66 +32:11:30.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 67090_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 67090_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 05:27:08.23 +30:12:30.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16231_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427
The candidate 16231_fd_Aur-05-Q1b1x1_2026-07-12_05-12-07_20.00sec_-0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 05:18:59.98 +33:44:51.9 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 4s
make_report_in_HTML.sh TOTAL: 48s
Prepared the HTML report for the field Aur-05-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
05:30:35.40 +32:47:41.9
05:26:51.35 +32:03:07.7
05:29:33.80 +29:20:53.6
05:33:29.32 +25:28:34.7
04:51:12.37 +25:58:31.7
05:08:43.29 +26:03:10.8
05:05:51.08 +26:46:29.3
05:18:31.28 +27:01:53.9
05:06:16.52 +27:22:15.4
04:59:57.74 +27:26:58.9
05:22:54.04 +27:26:39.4
05:02:50.79 +28:43:15.6
04:45:50.66 +28:10:28.4
05:06:18.62 +28:34:06.1
04:34:18.76 +30:23:06.6
05:32:21.08 +25:21:16.9
05:28:50.24 +33:29:34.2
05:33:05.21 +25:07:43.7
05:33:32.78 +25:43:15.4
05:19:44.27 +26:10:31.3
05:31:03.09 +24:58:11.2
05:20:40.99 +32:46:02.3
05:02:27.13 +32:51:56.9
05:01:05.18 +32:51:54.4
05:12:02.91 +32:26:56.3
05:01:11.29 +32:26:10.7
04:58:45.63 +32:09:05.0
05:06:14.13 +32:02:13.4
04:59:02.06 +31:50:19.3
05:16:23.38 +31:33:47.1
05:05:26.34 +31:29:49.7
04:53:30.35 +31:26:31.6
05:13:59.20 +31:03:18.6
04:45:17.75 +31:12:11.8
05:01:21.17 +30:48:07.8
05:07:49.51 +30:24:04.3
05:25:49.97 +30:05:45.3
04:38:07.76 +29:58:31.9
05:33:23.04 +29:29:45.3
05:06:29.74 +29:26:30.7
04:52:40.42 +29:13:59.8
05:07:35.82 +29:00:15.8
05:18:54.39 +25:01:24.8
05:20:58.54 +25:08:44.2
05:05:08.99 +25:22:10.4
########### Completed Aur-05-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
05:33:29.32 +25:28:34.7
05:29:33.80 +29:20:53.6
05:26:51.35 +32:03:07.7
05:30:35.40 +32:47:41.9
04:34:18.76 +30:23:06.6
05:32:21.08 +25:21:16.9
05:28:50.24 +33:29:34.2
05:33:05.21 +25:07:43.7
05:33:32.78 +25:43:15.4
05:19:44.27 +26:10:31.3
05:31:03.09 +24:58:11.2
04:45:17.75 +31:12:11.8
05:20:40.99 +32:46:02.3
04:52:40.42 +29:13:59.8
05:16:23.38 +31:33:47.1
05:01:05.18 +32:51:54.4
04:59:57.74 +27:26:58.9
05:20:58.54 +25:08:44.2
05:12:02.91 +32:26:56.3
05:05:08.99 +25:22:10.4
04:45:50.66 +28:10:28.4
04:58:45.63 +32:09:05.0
05:08:43.29 +26:03:10.8
05:07:35.82 +29:00:15.8
05:06:29.74 +29:26:30.7
04:53:30.35 +31:26:31.6
05:05:51.08 +26:46:29.3
05:02:50.79 +28:43:15.6
05:06:18.62 +28:34:06.1
05:01:21.17 +30:48:07.8
04:59:02.06 +31:50:19.3
05:18:31.28 +27:01:53.9
04:38:07.76 +29:58:31.9
05:06:14.13 +32:02:13.4
05:18:54.39 +25:01:24.8
05:22:54.04 +27:26:39.4
04:51:12.37 +25:58:31.7
05:01:11.29 +32:26:10.7
05:25:49.97 +30:05:45.3
05:02:27.13 +32:51:56.9
05:07:49.51 +30:24:04.3
05:06:16.52 +27:22:15.4
05:05:26.34 +31:29:49.7
05:33:23.04 +29:29:45.3
05:13:59.20 +31:03:18.6
###################################################################################
05:33:29.32 +25:28:34.7 -- not an asteroid (will add it to exclusion list)
05:29:33.80 +29:20:53.6 -- not an asteroid (will add it to exclusion list)
05:26:51.35 +32:03:07.7 -- not an asteroid (will add it to exclusion list)
05:30:35.40 +32:47:41.9 -- not an asteroid (will add it to exclusion list)
04:34:18.76 +30:23:06.6 -- asteroid (will NOT add it to exclusion list)
05:32:21.08 +25:21:16.9 -- not an asteroid (will add it to exclusion list)
05:28:50.24 +33:29:34.2 -- asteroid (will NOT add it to exclusion list)
05:33:05.21 +25:07:43.7 -- not an asteroid (will add it to exclusion list)
05:33:32.78 +25:43:15.4 -- not an asteroid (will add it to exclusion list)
05:19:44.27 +26:10:31.3 -- not an asteroid (will add it to exclusion list)
05:31:03.09 +24:58:11.2 -- not an asteroid (will add it to exclusion list)
04:45:17.75 +31:12:11.8 -- not an asteroid (will add it to exclusion list)
05:20:40.99 +32:46:02.3 -- not an asteroid (will add it to exclusion list)
04:52:40.42 +29:13:59.8 -- not an asteroid (will add it to exclusion list)
05:16:23.38 +31:33:47.1 -- not an asteroid (will add it to exclusion list)
05:01:05.18 +32:51:54.4 -- not an asteroid (will add it to exclusion list)
04:59:57.74 +27:26:58.9 -- not an asteroid (will add it to exclusion list)
05:20:58.54 +25:08:44.2 -- not an asteroid (will add it to exclusion list)
05:12:02.91 +32:26:56.3 -- not an asteroid (will add it to exclusion list)
05:05:08.99 +25:22:10.4 -- not an asteroid (will add it to exclusion list)
04:45:50.66 +28:10:28.4 -- not an asteroid (will add it to exclusion list)
04:58:45.63 +32:09:05.0 -- not an asteroid (will add it to exclusion list)
05:08:43.29 +26:03:10.8 -- not an asteroid (will add it to exclusion list)
05:07:35.82 +29:00:15.8 -- not an asteroid (will add it to exclusion list)
05:06:29.74 +29:26:30.7 -- not an asteroid (will add it to exclusion list)
04:53:30.35 +31:26:31.6 -- not an asteroid (will add it to exclusion list)
05:05:51.08 +26:46:29.3 -- not an asteroid (will add it to exclusion list)
05:02:50.79 +28:43:15.6 -- not an asteroid (will add it to exclusion list)
05:06:18.62 +28:34:06.1 -- not an asteroid (will add it to exclusion list)
05:01:21.17 +30:48:07.8 -- not an asteroid (will add it to exclusion list)
04:59:02.06 +31:50:19.3 -- not an asteroid (will add it to exclusion list)
05:18:31.28 +27:01:53.9 -- not an asteroid (will add it to exclusion list)
04:38:07.76 +29:58:31.9 -- not an asteroid (will add it to exclusion list)
05:06:14.13 +32:02:13.4 -- not an asteroid (will add it to exclusion list)
05:18:54.39 +25:01:24.8 -- not an asteroid (will add it to exclusion list)
05:22:54.04 +27:26:39.4 -- not an asteroid (will add it to exclusion list)
04:51:12.37 +25:58:31.7 -- not an asteroid (will add it to exclusion list)
05:01:11.29 +32:26:10.7 -- not an asteroid (will add it to exclusion list)
05:25:49.97 +30:05:45.3 -- not an asteroid (will add it to exclusion list)
05:02:27.13 +32:51:56.9 -- not an asteroid (will add it to exclusion list)
05:07:49.51 +30:24:04.3 -- not an asteroid (will add it to exclusion list)
05:06:16.52 +27:22:15.4 -- not an asteroid (will add it to exclusion list)
05:05:26.34 +31:29:49.7 -- not an asteroid (will add it to exclusion list)
05:33:23.04 +29:29:45.3 -- not an asteroid (will add it to exclusion list)
05:13:59.20 +31:03:18.6 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
04:38:07.76 +29:58:31.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:45:17.75 +31:12:11.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:45:50.66 +28:10:28.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:51:12.37 +25:58:31.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:52:40.42 +29:13:59.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:53:30.35 +31:26:31.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:45.63 +32:09:05.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:02.06 +31:50:19.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:57.74 +27:26:58.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:01:05.18 +32:51:54.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:01:11.29 +32:26:10.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:01:21.17 +30:48:07.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:02:27.13 +32:51:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:02:50.79 +28:43:15.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:05:08.99 +25:22:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:05:26.34 +31:29:49.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:05:51.08 +26:46:29.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:06:14.13 +32:02:13.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:06:16.52 +27:22:15.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:06:18.62 +28:34:06.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:06:29.74 +29:26:30.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:07:35.82 +29:00:15.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:07:49.51 +30:24:04.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:08:43.29 +26:03:10.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:12:02.91 +32:26:56.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:13:59.20 +31:03:18.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:16:23.38 +31:33:47.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:31.28 +27:01:53.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:54.39 +25:01:24.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:19:44.27 +26:10:31.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:20:40.99 +32:46:02.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:20:58.54 +25:08:44.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:22:54.04 +27:26:39.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:25:49.97 +30:05:45.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:26:51.35 +32:03:07.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:29:33.80 +29:20:53.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:30:35.40 +32:47:41.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:31:03.09 +24:58:11.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:32:21.08 +25:21:16.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:33:05.21 +25:07:43.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:33:23.04 +29:29:45.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:33:29.32 +25:28:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:33:32.78 +25:43:15.4 -- 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)
04:38:07.76 +29:58:31.9 -- a known variable star
04:45:17.75 +31:12:11.8 -- a known variable star
04:45:50.66 +28:10:28.4 -- a known variable star
04:51:12.37 +25:58:31.7 -- a known variable star
04:52:40.42 +29:13:59.8 -- not a known variable star
04:53:30.35 +31:26:31.6 -- a known variable star
04:58:45.63 +32:09:05.0 -- a known variable star
04:59:02.06 +31:50:19.3 -- a known variable star
04:59:57.74 +27:26:58.9 -- a known variable star
05:01:05.18 +32:51:54.4 -- a known variable star
05:01:11.29 +32:26:10.7 -- a known variable star
05:01:21.17 +30:48:07.8 -- a known variable star
05:02:27.13 +32:51:56.9 -- a known variable star
05:02:50.79 +28:43:15.6 -- a known variable star
05:05:08.99 +25:22:10.4 -- a known variable star
05:05:26.34 +31:29:49.7 -- a known variable star
05:05:51.08 +26:46:29.3 -- a known variable star
05:06:14.13 +32:02:13.4 -- a known variable star
05:06:16.52 +27:22:15.4 -- a known variable star
05:06:18.62 +28:34:06.1 -- a known variable star
05:06:29.74 +29:26:30.7 -- a known variable star
05:07:35.82 +29:00:15.8 -- a known variable star
05:07:49.51 +30:24:04.3 -- a known variable star
05:08:43.29 +26:03:10.8 -- a known variable star
05:12:02.91 +32:26:56.3 -- a known variable star
05:13:59.20 +31:03:18.6 -- a known variable star
05:16:23.38 +31:33:47.1 -- a known variable star
05:18:31.28 +27:01:53.9 -- a known variable star
05:18:54.39 +25:01:24.8 -- a known variable star
05:19:44.27 +26:10:31.3 -- a known variable star
05:20:40.99 +32:46:02.3 -- a known variable star
05:20:58.54 +25:08:44.2 -- a known variable star
05:22:54.04 +27:26:39.4 -- a known variable star
05:25:49.97 +30:05:45.3 -- a known variable star
05:26:51.35 +32:03:07.7 -- a known variable star
05:29:33.80 +29:20:53.6 -- a known variable star
05:30:35.40 +32:47:41.9 -- a known variable star
05:31:03.09 +24:58:11.2 -- not a known variable star
05:32:21.08 +25:21:16.9 -- a known variable star
05:33:05.21 +25:07:43.7 -- not a known variable star
05:33:23.04 +29:29:45.3 -- a known variable star
05:33:29.32 +25:28:34.7 -- not a known variable star
05:33:32.78 +25:43:15.4 -- not a known variable star
Found 5 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
43 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
###################################################################################
Adding identified Gaia sources from exclusion_list_gaiadr2.txt
exclusion_list_apass.txt NOT FOUND
IS_THIS_TEST_RUN= NO ALLOW_EXCLUSION_LIST_UPDATE= YES
#### Adding the following to the exclusion list ####
04:38:07.76 +29:58:31.9
04:45:17.75 +31:12:11.8
04:45:50.66 +28:10:28.4
04:51:12.37 +25:58:31.7
04:52:40.42 +29:13:59.8
04:53:30.35 +31:26:31.6
04:58:45.63 +32:09:05.0
04:59:02.06 +31:50:19.3
04:59:57.74 +27:26:58.9
05:01:05.18 +32:51:54.4
05:01:11.29 +32:26:10.7
05:01:21.17 +30:48:07.8
05:02:27.13 +32:51:56.9
05:02:50.79 +28:43:15.6
05:05:08.99 +25:22:10.4
05:05:26.34 +31:29:49.7
05:05:51.08 +26:46:29.3
05:06:14.13 +32:02:13.4
05:06:16.52 +27:22:15.4
05:06:18.62 +28:34:06.1
05:06:29.74 +29:26:30.7
05:07:35.82 +29:00:15.8
05:07:49.51 +30:24:04.3
05:08:43.29 +26:03:10.8
05:12:02.91 +32:26:56.3
05:13:59.20 +31:03:18.6
05:16:23.38 +31:33:47.1
05:18:31.28 +27:01:53.9
05:18:54.39 +25:01:24.8
05:19:44.27 +26:10:31.3
05:20:40.99 +32:46:02.3
05:20:58.54 +25:08:44.2
05:22:54.04 +27:26:39.4
05:25:49.97 +30:05:45.3
05:26:51.35 +32:03:07.7
05:29:33.80 +29:20:53.6
05:30:35.40 +32:47:41.9
05:31:03.09 +24:58:11.2
05:32:21.08 +25:21:16.9
05:33:05.21 +25:07:43.7
05:33:23.04 +29:29:45.3
05:33:29.32 +25:28:34.7
05:33:32.78 +25:43:15.4
04:40:28.16 +30:16:48.8
####################################################
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461233.92456365 -observatory V36
07:26:40.55 +17:05:57.9 Mercury (5.6mag)
10:20:17.85 +11:45:58.1 Venus (-4.1mag)
04:30:19.31 +21:40:23.0 Mars (1.3mag)
08:18:33.72 +20:05:30.5 Jupiter (-1.8mag)
00:56:03.81 +03:21:12.3 Saturn (0.7mag)
04:07:37.63 +20:46:07.0 Uranus (5.8mag)
00:17:00.68 +00:20:28.8 Neptune (7.7mag)
20:30:43.45 -23:18:55.5 Pluto (14.4mag)
05:26:19.15 +27:23:42.0 Moon (-8.8mag)
-rw-r--r-- 1 apache apache 361 Jul 12 07:40 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461233.92456365:
08:18:40.72 +20:05:04.4 Io (6.1mag)
08:18:28.59 +20:05:49.8 Europa (6.3mag)
08:18:35.22 +20:05:21.5 Ganymede (5.6mag)
08:18:46.69 +20:04:38.8 Callisto (6.8mag)
08:16:59.50 +19:50:32.8 Himalia (15.7mag)
08:18:34.37 +20:05:28.8 Thebe (16.6mag)
08:16:20.40 +19:54:33.4 Elara (17.6mag)
08:22:09.77 +19:58:34.0 Pasiphae (17.8mag)
08:23:24.45 +20:10:53.5 Carme (19.0mag)
00:56:01.72 +03:20:44.3 Titan (8.5mag)
00:56:08.74 +03:21:03.5 Rhea (9.8mag)
00:55:30.88 +03:19:57.7 Iapetus (11.2mag)
00:56:04.22 +03:21:41.6 Hyperion (14.5mag)
00:56:01.76 +03:18:07.9 Phoebe (16.6mag)
-rw-r--r-- 1 apache apache 568 Jul 12 07:40 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461233.92456365:
17:48:38.15 -32:29:48.1 JWST
12:33:51.71 +51:27:40.7 Chandra
05:43:40.73 +37:09:25.6 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jul 12 07:40 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461233.92456365 -observatory V36
02:39:12.69 +14:40:28.1 17.9mag P/1996 R2 (Lagerkvist)
18:16:21.17 -34:25:08.7 13.7mag P/2010 H2 (Vales)
06:27:45.04 -68:10:23.0 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:01:31.58 +32:28:56.5 17.6mag C/2017 K2 (PANSTARRS)
01:59:22.63 +12:11:35.4 15.5mag P/2021 N1 (ZTF)
22:58:16.80 +32:16:50.7 17.3mag C/2022 E2 (ATLAS)
06:14:45.88 +26:54:28.3 16.7mag C/2022 N2 (PANSTARRS)
09:57:19.36 +29:41:17.3 16.8mag C/2022 QE78 (ATLAS)
09:11:04.46 +05:02:19.0 17.8mag C/2022 R6 (PANSTARRS)
18:05:57.53 +21:12:48.4 18.0mag C/2023 A3 (Tsuchinshan-ATLAS)
15:11:23.28 -11:26:07.9 17.7mag P/2023 B1 (PANSTARRS)
21:46:43.50 +67:36:19.2 17.8mag C/2023 H5 (Lemmon)
16:26:49.79 -10:17:41.6 13.9mag C/2023 R1 (PANSTARRS)
08:04:15.07 +65:49:12.7 17.9mag C/2024 A1 (ATLAS)
07:35:31.78 +30:06:32.6 14.7mag C/2024 E1 (Wierzchos)
15:15:20.10 +15:22:55.3 17.6mag C/2024 G6 (ATLAS)
19:38:39.89 +39:47:39.5 13.8mag C/2024 J3 (ATLAS)
21:45:25.50 +46:18:48.9 17.8mag C/2024 R4 (PANSTARRS)
04:51:35.72 -13:42:09.9 15.7mag C/2024 T5 (ATLAS)
06:36:17.39 +28:43:27.3 18.0mag C/2025 J1 (Borisov)
07:15:47.46 -13:04:27.1 16.6mag C/2025 R3 (PANSTARRS)
09:58:30.10 +22:20:51.6 17.6mag C/2025 V2 (Rankin)
12:45:19.02 +03:50:55.6 17.1mag C/2025 Y1 (ATLAS)
16:46:07.87 +79:09:23.2 17.3mag C/2026 A2 (Bok)
02:48:27.93 +45:19:47.0 16.7mag C/2026 B2 (Sun-Gao)
11:26:50.22 +04:54:38.2 17.0mag A/2026 E1
21:22:16.85 -15:49:22.3 7.2mag 10P/Tempel
11:14:25.82 -01:58:34.0 16.2mag 29P/Schwassmann-Wachmann
04:03:09.62 +29:46:43.0 17.9mag 47P/Ashbrook-Jackson
10:12:24.54 +13:21:02.6 17.0mag 63P/Wild
00:49:15.12 -05:04:12.8 15.5mag 65P/Gunn
08:33:25.10 +34:06:54.7 18.0mag 76P/West-Kohoutek-Ikemura
04:32:24.86 +20:17:06.4 13.7mag 78P/Gehrels
02:25:40.95 +10:53:42.3 16.2mag 88P/Howell
06:41:42.13 +30:24:38.8 15.7mag 93P/Lovas
04:27:44.02 +31:12:24.2 16.8mag 114P/Wiseman-Skiff
08:13:45.86 +30:28:18.5 15.2mag 123P/West-Hartley
10:52:00.09 +00:20:36.6 16.8mag 124P/Mrkos
04:55:03.63 +20:52:19.0 16.2mag 128P/Shoemaker-Holt
05:40:10.05 +19:41:49.9 17.8mag 131P/Mueller
00:02:05.90 +03:00:55.5 17.9mag 139P/Vaisala-Oterma
07:21:11.20 +16:34:17.9 15.8mag 141P-D/Machholz
03:17:43.03 -20:56:02.1 15.4mag 161P/Hartley-IRAS
05:40:32.03 +34:23:29.8 15.4mag 162P/SidingSpring
18:59:01.18 +16:22:21.3 14.6mag 169P/NEAT
01:45:58.61 +07:49:49.8 17.7mag 220P/McNaught
16:35:42.36 -08:28:05.1 17.1mag 235P/LINEAR
08:49:39.42 +33:06:28.4 17.9mag 240P/NEAT
20:41:15.75 -50:01:16.9 17.8mag 259P/Garradd
02:05:06.68 +13:03:54.4 15.7mag 260P/McNaught
05:43:31.10 +37:00:26.3 17.4mag 295P/LINEAR
15:06:30.91 +05:52:19.0 17.6mag 391P/Kowalski
08:36:27.99 +19:35:33.2 17.9mag 450P/LONEOS
07:55:01.42 +39:02:38.8 17.9mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.7K Jul 12 07:40 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
11:06:55.46 -04:07:04.50 AT2026qqg 2026-07-5.01 16.82
19:07:23.69 -74:13:37.30 AT2026qly 2026-07-5.02 17.31
17:57:43.80 +27:18:40.10 ASASSN-26ea 2026-07-5.07 16.67
19:59:01.43 -32:07:34.30 ASASSN-26eb 2026-07-4.97 15.52
18:46:50.35 -57:44:13.20 SN 2026qqp 2026-07-5.03 -0.92
19:17:31.69 -39:55:29.90 ASASSN-26dz 2026-07-5.14 15.91
19:14:31.37 +12:03:52.90 AT 2026rdg 2026-07-3.43 11.81
04:05:50.09 -70:24:34.40 AT 2026qpr 2026-06-30.4 15.96
13:45:37.49 -05:59:35.80 SN 2026pub 2026-06-30.09 16.01
16:41:15.63 +39:17:14.70 SN 2026pel 2026-06-26.38 16.07
10:14:40.19 -35:38:21.30 ASASSN-26dy 2026-06-25.99 15.63
14:47:21.56 -40:15:51.30 ASASSN-26dv 2026-06-23.03 14.62
13:38:49.79 -77:21:06.70 ASASSN-26dw 2026-06-23.04 16.09
00:59:27.90 +33:08:13.20 SN 2026mke 2026-06-22.39 17.13
11:10:44.73 -30:20:45.50 SN 2026nmv 2026-06-22.06 16.56
21:36:15.68 -21:19:12.50 AT2026oxh 2026-06-22.15 17.14
17:31:38.38 -56:05:51.90 ASASSN-26dx 2026-06-22.02 14.72
14:10:13.44 -38:46:46.10 AT2026pvk 2026-06-22.06 16.53
20:56:47.23 -18:31:05.20 AT2026plb 2026-06-21.31 16.4
15:44:29.68 +21:00:59.30 SN2026ore 2026-06-21.29 17.57
23:50:05.98 -14:01:41.30 AT2026oxl 2026-06-21.52 17.64
17:36:54.73 -18:10:04.20 AT2026ouj 2026-06-20.92 15.15
00:34:04.08 -30:22:09.20 AT2026ntk 2026-06-18.09 17.34
20:49:13.39 +25:17:59.20 ASASSN-26du 2026-06-15.39 15.93
23:09:30.84 +32:40:42.00 SN2026oxc 2026-06-14.35 16.83
02:02:26.78 +32:04:21.30 AT2026ovz 2026-06-14.59 15.39
21:26:28.11 -72:31:19.50 AT2026nwc 2026-06-11 17.05
17:54:57.33 +26:32:34.20 SN 2026odc 2026-06-11.23 17.62
13:55:59.94 +17:30:37.20 SN 2026nyq 2026-06-11.1 16.24
00:50:45.14 -71:38:36.90 ASASSN-26dt 2026-06-11.13 10.22
14:42:19.73 +19:11:35.60 SN2026nyp 2026-06-10.3 16.32
12:23:23.92 +12:56:43.50 SN2026mta 2026-06-8.29 16.69
12:30:18.51 +47:12:33.20 SN2026oao 2026-06-9.32 17.02
10:51:05.21 -42:28:56.60 AT2026nvf 2026-06-8.12 16.75
13:50:22.48 -07:35:00.00 SN2026npn 2026-06-8.02 17.58
00:56:07.17 +43:01:43.20 ASASSN-26dq 2026-06-7.43 13.58
01:07:49.46 +41:59:43.70 SN 2026obc 2026-06-7.43 15.15
21:11:25.22 +14:14:31.90 ASASSN-26dr 2026-06-7.24 16.24
06:21:27.06 -65:16:42.00 ASASSN-26ds 2026-06-2.97 15.02
20:07:38.15 -21:07:05.40 SN2026mho 2026-05-25.18 -1.12
11:29:42.55 +79:01:03.10 AT2026min 2026-05-24.21 16.63
11:44:33.11 -68:48:32.90 ASASSN-26no 2026-05-24.03 8.35
19:00:42.82 -48:31:01.60 ASASSN-26dp 2026-05-22.31 -3.28
14:23:56.72 -58:37:47.60 ASASSN-26dn 2026-05-20.01 14.64
11:24:54.06 +47:57:01.60 AT2026nma 2026-05-20.29 15.46
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
15:16:06.61 -79:16:32.40 ASASSN-26dm 2026-05-19.03 14.44
11:24:25.21 -59:23:19.10 ASASSN-26dl 2026-05-18.02 13.55
13:45:51.52 -53:16:01.00 ASASSN-26dk 2026-05-18.16 12.96
02:05:49.69 -30:29:09.60 ASASSN-26dh 2026-05-18.43 15.37
17:50:22.87 -39:42:33.90 ASASSN-26dj 2026-05-17.05 15.7
01:13:11.60 -33:25:16.10 ASASSN-26dg 2026-05-13.41 16.8
16:44:31.77 -27:15:18.40 AT2026mhn 2026-05-12.33 15.8
09:46:31.08 -33:41:51.00 ASASSN-26di 2026-05-12.14 14.63
21:23:11.57 -19:09:45.00 AT2026kwu 2026-05-12.26 16.9
14:20:14.30 -30:20:51.90 AT2026ktm 2026-05-12.06 17.21
14:41:39.01 -37:13:46.40 AT2026lkm 2026-05-11.18 16.89
12:59:50.45 -10:58:38.80 SN2026kep 2026-05-9.06 17.5
13:37:29.61 -29:50:30.90 AT2026lkd 2026-05-9.09 17.23
09:46:42.01 -14:52:03.60 SN2026kmo 2026-05-8.99 17.51
15:03:05.28 +22:02:03.80 AT2026lxf 2026-05-8.34 13.72
10:23:49.41 -20:57:25.30 ASASSN-26df 2026-05-8.21 16.52
22:14:40.56 +05:04:51.60 2026lda 2026-05-7.56 16.2
21:35:33.81 -14:05:16.30 ASASSN-26de 2026-05-6.29 14.51
16:21:48.82 -61:36:13.20 ASASSN-26dd 2026-05-5.21 15.15
14:26:40.22 -24:48:37.50 AT2026lig 2026-05-4.27 14.63
13:17:51.04 +30:25:13.50 SN2026kcp 2026-05-4.46 16.43
11:27:55.57 -13:38:56.90 SN2026kza 2026-05-1.08 15.59
22:28:27.10 +30:17:54.30 SN 2026fov 2026-04-29.6 14.36
21:00:10.71 -32:17:03.90 AT2026kis 2026-04-27.36 16.15
14:32:57.37 -58:13:26.40 ASASSN-26dc 2026-04-27.27 13.42
15:32:05.35 -43:54:34.60 ASASSN-26db 2026-04-27.37 16.06
16:34:34.97 -54:34:58.00 ASASSN-26da 2026-04-25.32 16.11
10:06:55.04 -01:13:49.70 SN2026jsg 2026-04-24.99 16.28
15:15:57.17 +56:18:32.80 SN2026kid 2026-04-24.52 -3.65
07:58:28.45 +57:03:42.40 AT2026kcf 2026-04-24.2 16.89
11:38:21.80 -50:43:06.50 SN2026jkb 2026-04-24.24 15.38
10:06:11.41 -39:41:04.20 AT2026dil 2026-04-24.2 16.85
14:21:40.08 +13:13:46.30 SN2026jlm 2026-04-22.16 15.12
10:53:55.47 -16:06:07.00 ASASSN-26cz 2026-04-22.24 16.32
11:06:55.46 -04:07:04.50 2026-07-5.01 16.82
13:45:02.03 +15:17:14.50 ASASSN-26cy 2026-04-21.27 15.78
13:20:52.22 -35:57:03.60 AT2026jcm 2026-04-19.01 16.65
13:36:15.66 -36:53:48.40 SN 2026iqy 2026-04-18.92 17.31
06:34:01.33 -40:07:34.00 ASASSN-26cx 2026-04-19.07 16.16
23:33:57.97 -45:12:11.90 SN 2026idu 2026-04-19.41 15.9
12:10:50.92 +66:55:31.20 SN 2026icv 2026-04-17.14 16.03
21:36:59.06 -60:43:35.90 ASASSN-26cv 2026-04-17.35 -1.18
08:13:26.26 -27:07:30.50 ASASSN-26cw 2026-04-17.07 -1.01
14:49:14.13 -27:29:20.60 ASASSN-26cu 2026-04-16.06 14.03
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
11:06:55.46 -04:07:04.50 2026-07-5.01 16.82
12:23:20.40 +04:53:39.10 AT2026ixd 2026-04-12.14 17.65
17:46:09.76 -61:19:50.40 SN2026icy 2026-04-12.2 17.03
09:25:46.42 +02:13:46.30 SN2026gud 2026-04-11.98 16.49
16:52:15.46 -60:27:45.90 ASASSN-26cs 2026-04-12.4 15.5
04:20:55.37 -51:15:31.10 ASASSN-26cr 2026-04-12.01 15.37
22:25:39.35 +36:45:06.90 AT2026ihl 2026-04-10.48 14.21
-rw-r--r-- 1 apache apache 5.6K Jul 12 07:40 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
00:43:35.02 +41:46:28.0 PNV J00433502+4146280 2026-04-23.056 15.9mag
00:42:55.64 +41:14:12.2 PNV J00425564+4114122 2026-04-24.042 16.2mag
21:14:03.38 +56:46:44.1 TCP J21140338+5646441 2026-05-05.3534 16.7mag
15:03:05.19 +22:02:04.1 TCP J15030519+2202041 2026-05-08.3260 13.9mag
07:15:18.25 +47:53:16.7 TCP J07151825+4753167 2026-05-09.1599 14.4mag
16:00:18.44 -22:30:10.6 TCP J16001844-2230106 2026-05-09.6135 13.3mag
00:42:47.45 +41:16:58.5 PNV J00424745+4116585 2026-05-10.030 16.8mag
09:55:02.89 +69:02:13.8 PNV J09550289+6902138 2026-05-18.925 20.7mag
00:43:01.82 +41:18:16.6 PNV J00430182+4118166 2026-05-21.8651 18.83Cmag
00:42:51.20 +41:16:59.4 PNV J00425120+4116594 2022-10-26.135 19.3mag
12:24:25.10 +28:47:12.0 TCP J12242510+2847120 2026-05-31.6015 14.8mag
00:56:07.13 +43:01:40.6 TCP J00560713+4301406 2026-06-01.4135 12.2mag
00:42:41.64 +41:15:16.2 PNV J00424164+4115162 2026-06-02.029 17.4mag
00:42:38.68 +41:15:58.2 PNV J00423868+4115582 2026-06-05.1224 19.97Umag
19:00:42.95 -48:31:01.7 PNV J19004295-4831017 2026-05-25.0752 14.2mag
09:55:21.28 +69:02:52.6 PNV J09552128+6902526 2026-06-13.933 18.9mag
19:51:21.42 +37:06:40.0 TCP J19512142+3706400 2026-06-17.2942 16.8mag
19:57:03.87 +37:41:46.4 TCP J19570387+3741464 2026-06-18.2638 17.5mag
00:42:32.04 +41:10:28.3 PNV J00423204+4110283 2026-06-26.059 16.6mag
-rw-r--r-- 1 apache apache 189K Jul 12 07:40 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
21:14:45.766 -17:59:34.07 AT 2026tfs 2026-07-07.32 23.3748
20:53:56.433 -20:10:29.29 AT 2026tfr 2026-07-07.33 21.8847
22:06:01.400 -08:26:04.36 AT 2026tfq 2026-07-07.42 22.8925
20:24:31.143 -19:57:10.94 AT 2026tfp 2026-07-07.33 22.5869
20:57:00.828 -22:33:31.10 AT 2026tfo 2026-07-07.32 22.5975
20:22:57.382 -27:32:12.84 AT 2026tfn 2026-07-07.34 23.1894
21:07:56.442 -20:11:00.78 AT 2026tfm 2026-07-07.32 22.5462
21:03:37.712 -19:23:03.02 AT 2026tfl 2026-07-07.33 23.0422
21:27:05.435 -20:41:33.13 AT 2026tfk 2026-07-07.40 23.0646
21:14:27.901 -20:03:56.28 AT 2026tfj 2026-07-07.32 22.4848
20:13:02.531 -18:35:56.09 AT 2026tfi 2026-07-06.29 22.9464
19:50:43.854 -14:18:25.75 AT 2026tfh 2026-07-06.29 22.6393
19:49:01.219 -14:39:02.57 AT 2026tfg 2026-07-06.29 23.097
19:22:24.530 -22:23:54.02 AT 2026tff 2026-07-06.24 21.7866
19:52:00.093 -27:46:43.92 AT 2026tfe 2026-07-06.28 22.4003
20:18:07.239 -18:25:09.68 AT 2026tfd 2026-07-06.29 22.9481
19:25:35.747 -20:22:41.48 AT 2026tfc 2026-07-06.27 22.9318
04:04:17.348 -47:13:16.79 AT 2026tfb 2026-07-06.42 22.8233
19:59:28.620 -13:56:29.91 AT 2026tfa 2026-07-06.29 22.0828
19:21:29.220 -18:09:15.97 AT 2026tez 2026-07-06.27 22.8329
-rw-r--r-- 1 apache apache 30K Jul 12 07:40 tns_transients_list.txt
