This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q1b1x1_055948_TTUQ1b1x1_572930_wIJUi5vl
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 12.4269 2461233.9269 10.60 05:47:32.85 +39:27:53.1
171.17759 5.78261 galactic Aur Second-epoch detections are separated by 0.5" and 3.3 pix
The object was found in VSX 1" NSVS J0547329+392753
Type: L:
# Max. Min./Amp. JD0 Period
10.131 R1 Y 0.355 R1 83.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:47:32.85 +39:27:53.1: 11.55 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:47:32.85 +39:27:53.1: 11.58 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.57 +/- 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 J0547329+392753,2461233.9269,10.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0547329+392753 20260712.4269 10.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4269 2461233.9269 9.90 05:20:55.63 +35:05:21.4
171.99178 -1.03485 galactic Aur Second-epoch detections are separated by 0.4" and 3.3 pix
The object was found in VSX 2" EE Aur
Type: LB
# Max. Min./Amp. JD0 Period
13.900 pg 15.500 pg M3-M7
ATTENTION: measured mag 9.90 is 4.0 mag brighter than the VSX record maximum brightness 13.90 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:20:55.63 +35:05:21.4: 11.36 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:20:55.63 +35:05:21.4: 10.95 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.09 +/- 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
EE Aur,2461233.9269,9.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
EE Aur 20260712.4269 9.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4269 2461233.9269 9.98 05:41:55.89 +38:56:00.6
171.06955 4.57662 galactic Aur Second-epoch detections are separated by 0.9" and 3.2 pix
The object was found in VSX 1" SZ Aur
Type: M
# Max. Min./Amp. JD0 Period
8.500 V 15.800 V 2439048.00000 456.400000000000 M8e
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:41:55.89 +38:56:00.6: 11.34 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:41:55.89 +38:56:00.6: 12.08 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.52 +/- 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!
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
SZ Aur,2461233.9269,9.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
SZ Aur 20260712.4269 9.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4269 2461233.9269 10.34 05:18:19.01 +35:14:59.8
171.55443 -1.38009 galactic Aur Second-epoch detections are separated by 0.4" and 3.3 pix
The object was found in VSX 0" DY Aur
Type: M
# Max. Min./Amp. JD0 Period
12.400 V 15.600 V 2441213.00000 473.840000000000 C(R)
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:18:19.01 +35:14:59.8: 12.48 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:18:19.01 +35:14:59.8: 12.22 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.32 +/- 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
DY Aur,2461233.9269,10.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DY Aur 20260712.4269 10.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4269 2461233.9269 10.92 05:10:20.38 +39:49:22.9
166.91968 0.01038 galactic Aur Second-epoch detections are separated by 0.2" and 3.1 pix
The object was found in VSX 1" V0480 Aur
Type: SR:
# Max. Min./Amp. JD0 Period
11.700 pg 13.200 pg 50.000000000000 C(N)
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:10:20.38 +39:49:22.9: 11.92 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:10:20.38 +39:49:22.9: 12.01 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.96 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0480 Aur,2461233.9269,10.92,0.05,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
V0480 Aur 20260712.4269 10.92CV 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 12.4269 2461233.9269 10.38 05:57:29.31 +41:11:02.9
170.62532 8.28159 galactic Aur Second-epoch detections are separated by 1.0" and 3.4 pix
The object was found in VSX 1" GSC 02916-00275
Type: SR
# Max. Min./Amp. JD0 Period
11.810 V Y 0.600 w 2456398.00000 141.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:57:29.31 +41:11:02.9: 11.29 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:57:29.31 +41:11:02.9: 11.38 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.33 +/- 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
GSC 02916-00275,2461233.9269,10.38,0.05,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
GSC 02916-00275 20260712.4269 10.38CV 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 12.4269 2461233.9269 10.79 05:21:01.14 +38:28:04.6
169.22626 0.90637 galactic Aur Second-epoch detections are separated by 1.1" and 3.2 pix
The object was found in VSX 2" DZ Aur
Type: LB
# Max. Min./Amp. JD0 Period
14.300 pg 15.500 pg M6
ATTENTION: measured mag 10.79 is 3.5 mag brighter than the VSX record maximum brightness 14.30 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:21:01.14 +38:28:04.6: 12.08 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:21:01.14 +38:28:04.6: 11.97 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.02 +/- 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
DZ Aur,2461233.9269,10.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DZ Aur 20260712.4269 10.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4269 2461233.9269 11.69 05:28:50.48 +33:29:34.1
174.23092 -0.57925 galactic Aur Second-epoch detections are separated by 1.2" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.89 Julia -1 0 1 11.5 0 0
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:28:50.48 +33:29:34.1: 15.28 +/- 0.24 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:28:50.48 +33:29:34.1: 14.80 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.93 +/- 0.13
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,2461233.9269,11.69,0.05,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 20260712.4269 11.69CV 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 12.4269 2461233.9269 11.70 05:30:18.67 +38:59:30.7
169.80638 2.70141 galactic Aur Second-epoch detections are separated by 0.5" and 3.4 pix
The object was found in VSX 0" ASASSN-V J053018.66+385931.1
Type: SR
# Max. Min./Amp. JD0 Period
12.620 V 13.690 V 2457980.10000 84.300000000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:30:18.67 +38:59:30.7: 13.06 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:30:18.67 +38:59:30.7: 12.72 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.82 +/- 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 J053018.66+385931.1,2461233.9269,11.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J053018.66+385931.1 20260712.4269 11.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4269 2461233.9269 12.14 05:45:01.83 +38:39:41.0
171.61791 4.95080 galactic Aur Second-epoch detections are separated by 1.0" and 3.3 pix
The object was found in VSX 1" V0735 Aur
Type: LB
# Max. Min./Amp. JD0 Period
11.350 R1 11.600 R1
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:45:01.83 +38:39:41.0: 13.36 +/- 0.03 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:45:01.83 +38:39:41.0: 13.11 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0735 Aur,2461233.9269,12.14,0.05,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
V0735 Aur 20260712.4269 12.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4269 2461233.9269 13.04 05:24:50.75 +36:46:09.0
171.05583 0.56991 galactic Aur Second-epoch detections are separated by 1.8" and 3.4 pix
The object was found in VSX 1" ASASSN-V J052450.83+364609.8
Type: SR
# Max. Min./Amp. JD0 Period
14.290 V 14.670 V 2457264.10000 69.700000000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:24:50.75 +36:46:09.0: 13.99 +/- 0.05 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:24:50.75 +36:46:09.0: 14.07 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.03 +/- 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 J052450.83+364609.8,2461233.9269,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J052450.83+364609.8 20260712.4269 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4269 2461233.9269 11.42 05:28:37.29 +34:02:29.4
173.74872 -0.31346 galactic Aur Second-epoch detections are separated by 1.6" and 3.5 pix
The object was found in VSX 1" NSVS J0528375+340228
Type: SR
# Max. Min./Amp. JD0 Period
14.367 g Y 0.532 g 2458430.01530 101.251128700000 MS
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:28:37.29 +34:02:29.4: 12.63 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:28:37.29 +34:02:29.4: 12.57 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.60 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin 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 J0528375+340228,2461233.9269,11.42,0.05,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
NSVS J0528375+340228 20260712.4269 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 12.4269 2461233.9269 11.52 05:10:09.13 +36:56:11.9
169.22106 -1.73256 galactic Aur Second-epoch detections are separated by 2.4" and 3.1 pix
The object was found in VSX 2" DR Aur
Type: SRA
# Max. Min./Amp. JD0 Period
14.600 pg 16.000 pg 2425991.00000 278.000000000000 M6
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:10:09.13 +36:56:11.9: 12.62 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:10:09.13 +36:56:11.9: 12.53 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.57 +/- 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
DR Aur,2461233.9269,11.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DR Aur 20260712.4269 11.52CV 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 12.4269 2461233.9269 12.14 05:37:30.83 +35:17:00.7
173.70343 1.89643 galactic Aur Second-epoch detections are separated by 1.6" and 3.6 pix
The object was found in VSX 3" ASASSN-V J053731.06+351701.4
Type: SR
# Max. Min./Amp. JD0 Period
15.300 g Y 0.830 g 2458402.83200
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:37:30.83 +35:17:00.7: 13.31 +/- 0.03 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:37:30.83 +35:17:00.7: 13.33 +/- 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!
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 J053731.06+351701.4,2461233.9269,12.14,0.05,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 J053731.06+351701.4 20260712.4269 12.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4269 2461233.9269 11.78 05:17:46.91 +36:59:31.6
170.06821 -0.46435 galactic Aur Second-epoch detections are separated by 1.5" and 3.5 pix
The object was found in VSX 2" V0486 Aur
Type: SR:
# Max. Min./Amp. JD0 Period
12.500 pg 13.600 pg 277.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:17:46.91 +36:59:31.6: 12.58 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:17:46.91 +36:59:31.6: 13.15 +/- 0.02 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
V0486 Aur,2461233.9269,11.78,0.05,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
V0486 Aur 20260712.4269 11.78CV 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 12.4269 2461233.9269 11.99 05:24:55.85 +40:04:01.8
168.33471 2.43493 galactic Aur Second-epoch detections are separated by 1.4" and 3.4 pix
The object was found in VSX 0" NEV45
Type: SRA
# Max. Min./Amp. JD0 Period
11.700 : V 14.200 : V 2457744.00000 453.000000000000 C
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:24:55.85 +40:04:01.8: 13.49 +/- 0.04 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:24:55.85 +40:04:01.8: 13.66 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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
NEV45,2461233.9269,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NEV45 20260712.4269 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4269 2461233.9269 11.21 05:06:30.50 +35:23:18.1
170.02477 -3.24692 galactic Aur Second-epoch detections are separated by 1.8" and 3.3 pix
The object was found in VSX 3" AQ Aur
Type: M
# Max. Min./Amp. JD0 Period
10.300 V 15.500 V 2454791.00000 343.000000000000 M7
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:06:30.50 +35:23:18.1: 12.55 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:06:30.50 +35:23:18.1: 13.23 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.72 +/- 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
AQ Aur,2461233.9269,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
AQ Aur 20260712.4269 11.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4269 2461233.9269 12.51 05:00:49.35 +34:37:49.6
169.92142 -4.63229 galactic Aur Second-epoch detections are separated by 1.2" and 3.3 pix
The object was found in VSX 4" ASASSN-V J050049.56+343752.3
Type: SR
# Max. Min./Amp. JD0 Period
14.150 V 14.970 V 2458588.30350 89.124492900000
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:00:49.35 +34:37:49.6: 13.51 +/- 0.04 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:00:49.35 +34:37:49.6: 13.42 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.46 +/- 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 J050049.56+343752.3,2461233.9269,12.51,0.05,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 J050049.56+343752.3 20260712.4269 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4269 2461233.9269 12.86 05:32:06.00 +41:17:38.6
168.06163 4.24547 galactic Aur Second-epoch detections are separated by 0.9" and 3.4 pix
The object was found in VSX 4" ASASSN-V J053205.69+411737.6
Type: SR
# Max. Min./Amp. JD0 Period
14.410 V 15.280 V 2458462.88650 221.719283800000
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:32:06.00 +41:17:38.6: 14.08 +/- 0.06 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:32:06.00 +41:17:38.6: 13.94 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.00 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J053205.69+411737.6,2461233.9269,12.86,0.05,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 J053205.69+411737.6 20260712.4269 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 12.4269 2461233.9269 11.54 04:59:47.65 +35:03:04.6
169.45813 -4.54090 galactic Aur Second-epoch detections are separated by 0.8" and 3.3 pix
The object was found in VSX 5" V0472 Aur
Type: SR:
# Max. Min./Amp. JD0 Period
12.800 pg 14.100 pg 199.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 04:59:47.65 +35:03:04.6: 12.99 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 04:59:47.65 +35:03:04.6: 12.40 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.55 +/- 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
V0472 Aur,2461233.9269,11.54,0.05,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
V0472 Aur 20260712.4269 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 12.4269 2461233.9269 12.86 05:16:15.54 +34:27:17.1
171.95994 -2.18401 galactic Aur Second-epoch detections are separated by 1.2" and 3.4 pix
The object was found in VSX 2" ZTF J051615.64+342715.8
Type: SR
# Max. Min./Amp. JD0 Period
15.260 g Y 0.223 g 2458457.76200 90.880355600000
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:16:15.54 +34:27:17.1: 13.84 +/- 0.05 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:16:15.54 +34:27:17.1: 13.78 +/- 0.05 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 J051615.64+342715.8,2461233.9269,12.86,0.05,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
ZTF J051615.64+342715.8 20260712.4269 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 12.4269 2461233.9269 12.84 05:08:17.26 +37:24:54.1
168.61530 -1.74599 galactic Aur Second-epoch detections are separated by 1.2" and 3.3 pix
The object was found in VSX 1" NSVS 6856406
Type: SR
# Max. Min./Amp. JD0 Period
13.244 r Y 0.980 r 2458483.89810 382.541714500000 C
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:08:17.26 +37:24:54.1: 14.10 +/- 0.06 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:08:17.26 +37:24:54.1: 14.33 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.19 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 6856406,2461233.9269,12.84,0.05,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
NSVS 6856406 20260712.4269 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 12.4269 2461233.9269 12.95 05:13:11.52 +33:50:57.0
172.08260 -3.05253 galactic Aur Second-epoch detections are separated by 2.0" and 3.1 pix
The object was found in VSX 2" NSVS J0513113+335055
Type: SR
# Max. Min./Amp. JD0 Period
13.705 r Y 0.956 r 2458309.31170 345.209866600000
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:13:11.52 +33:50:57.0: 14.41 +/- 0.08 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:13:11.52 +33:50:57.0: 13.91 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.06 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0513113+335055,2461233.9269,12.95,0.05,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 J0513113+335055 20260712.4269 12.95CV 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 12.4269 2461233.9269 12.16 05:32:02.40 +38:38:23.6
170.28582 2.79061 galactic Aur Second-epoch detections are separated by 2.4" and 3.6 pix
The object was found in VSX10" NSVS J0532032+383822
Type: L
# Max. Min./Amp. JD0 Period
11.175 R1 Y 0.471 R1 426.000000000000 C
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:32:02.40 +38:38:23.6: 13.62 +/- 0.04 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:32:02.40 +38:38:23.6: 13.35 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0532032+383822,2461233.9269,12.16,0.05,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
NSVS J0532032+383822 20260712.4269 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 12.4269 2461233.9269 11.19 05:40:07.75 +37:38:11.5
171.98893 3.59363 galactic Aur Second-epoch detections are separated by 2.1" and 3.4 pix
The object was found in VSX 2" RU Aur
Type: M
# Max. Min./Amp. JD0 Period
8.000 V 16.500 V 2458540.00000 469.500000000000 M7e-M9e
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:40:07.75 +37:38:11.5: 12.10 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:40:07.75 +37:38:11.5: 12.83 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.32 +/- 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!
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
RU Aur,2461233.9269,11.19,0.05,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
RU Aur 20260712.4269 11.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4269 2461233.9269 12.04 05:17:30.61 +34:49:22.4
171.80836 -1.76116 galactic Aur Second-epoch detections are separated by 0.6" and 3.4 pix
The object was found in VSX 2" ASASSN-V J051730.48+344920.2
Type: SR
# Max. Min./Amp. JD0 Period
13.530 V 13.960 V 2458205.27960 53.329493300000
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:17:30.61 +34:49:22.4: 13.19 +/- 0.03 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:17:30.61 +34:49:22.4: 13.08 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.13 +/- 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 J051730.48+344920.2,2461233.9269,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J051730.48+344920.2 20260712.4269 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4269 2461233.9269 11.94 05:26:35.54 +35:15:11.6
172.50956 0.01354 galactic Aur Second-epoch detections are separated by 1.4" and 3.5 pix
The object was found in VSX 4" NSVS J0526353+351509
Type: L:
# Max. Min./Amp. JD0 Period
11.218 R1 Y 0.271 R1 353.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:26:35.54 +35:15:11.6: 13.24 +/- 0.03 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:26:35.54 +35:15:11.6: 13.12 +/- 0.02 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
NSVS J0526353+351509,2461233.9269,11.94,0.05,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 J0526353+351509 20260712.4269 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4269 2461233.9269 12.78 05:31:11.28 +37:20:50.9
171.27699 1.94340 galactic Aur Second-epoch detections are separated by 3.2" and 3.8 pix
The object was found in VSX 0" NSVS J0531116+372048
Type: SR
# Max. Min./Amp. JD0 Period
16.329 g Y 0.384 g 2458579.93200 393.714434000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:31:11.28 +37:20:50.9: 14.20 +/- 0.06 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:31:11.28 +37:20:50.9: 14.39 +/- 0.07 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
NSVS J0531116+372048,2461233.9269,12.78,0.05,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 J0531116+372048 20260712.4269 12.78CV 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 12.4269 2461233.9269 12.38 05:03:20.33 +36:34:50.8
168.68524 -3.03726 galactic Aur Second-epoch detections are separated by 0.7" and 3.1 pix
The object was found in VSX 1" ASASSN-V J050320.27+363451.2
Type: SR
# Max. Min./Amp. JD0 Period
14.160 V 14.720 V 2458392.64440 126.047004100000
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:03:20.33 +36:34:50.8: 14.08 +/- 0.06 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:03:20.33 +36:34:50.8: 13.51 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J050320.27+363451.2,2461233.9269,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J050320.27+363451.2 20260712.4269 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4269 2461233.9269 12.22 05:30:24.07 +39:15:41.2
169.59037 2.86399 galactic Aur Second-epoch detections are separated by 0.9" and 3.4 pix
The object was found in VSX 3" V0491 Aur
Type: LB:
# Max. Min./Amp. JD0 Period
13.700 pg 15.000 pg
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:30:24.07 +39:15:41.2: 13.31 +/- 0.03 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:30:24.07 +39:15:41.2: 13.07 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0491 Aur,2461233.9269,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0491 Aur 20260712.4269 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4269 2461233.9269 12.56 05:20:58.41 +35:48:43.1
171.40333 -0.61512 galactic Aur Second-epoch detections are separated by 2.2" and 3.4 pix
The object was found in VSX 2" ZTF J052058.51+354842.0
Type: SR
# Max. Min./Amp. JD0 Period
15.469 g Y 0.265 g 2458560.68800 59.305954500000
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:20:58.41 +35:48:43.1: 13.84 +/- 0.05 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:20:58.41 +35:48:43.1: 13.71 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.77 +/- 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 J052058.51+354842.0,2461233.9269,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J052058.51+354842.0 20260712.4269 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4269 2461233.9269 12.18 05:40:58.91 +38:58:51.0
170.93200 4.44425 galactic Aur Second-epoch detections are separated by 1.1" and 3.2 pix
The object was found in VSX 1" ASASSN-V J054058.85+385851.4
Type: L
# Max. Min./Amp. JD0 Period
13.220 V 13.800 V
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:40:58.91 +38:58:51.0: 13.13 +/- 0.03 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:40:58.91 +38:58:51.0: 13.24 +/- 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 J054058.85+385851.4,2461233.9269,12.18,0.05,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 J054058.85+385851.4 20260712.4269 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 12.4269 2461233.9269 11.23 05:46:54.87 +41:24:30.6
169.43355 6.66965 galactic Aur Second-epoch detections are separated by 1.0" and 3.2 pix
The object was found in VSX 0" NSVS 4521908
Type: SR
# Max. Min./Amp. JD0 Period
13.752 g Y 0.529 g 2458378.64490 440.668594100000
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:46:54.87 +41:24:30.6: 12.43 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:46:54.87 +41:24:30.6: 12.17 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.27 +/- 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 4521908,2461233.9269,11.23,0.05,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 4521908 20260712.4269 11.23CV 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 12.4269 2461233.9269 12.88 05:16:02.97 +35:53:46.6
170.76029 -1.38271 galactic Aur Second-epoch detections are separated by 3.8" and 3.1 pix
The object was found in VSX 1" ASASSN-V J051603.01+355345.4
Type: SR
# Max. Min./Amp. JD0 Period
14.220 V 14.490 V 2458355.90390 41.046899300000
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:16:02.97 +35:53:46.6: 13.95 +/- 0.05 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:16:02.97 +35:53:46.6: 13.83 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.89 +/- 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 J051603.01+355345.4,2461233.9269,12.88,0.05,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 J051603.01+355345.4 20260712.4269 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4269 2461233.9269 12.24 05:23:15.74 +33:32:07.8
173.54519 -1.51947 galactic Aur Second-epoch detections are separated by 1.1" and 3.4 pix
The object was found in VSX 1" GSC 02394-01466
Type: SRB
# Max. Min./Amp. JD0 Period
13.600 V 14.200 V 2457458.50000 104.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:23:15.74 +33:32:07.8: 13.38 +/- 0.04 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:23:15.74 +33:32:07.8: 13.20 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.27 +/- 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
GSC 02394-01466,2461233.9269,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GSC 02394-01466 20260712.4269 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4269 2461233.9269 12.03 05:26:53.89 +35:34:49.3
172.27283 0.24776 galactic Aur Second-epoch detections are separated by 1.3" and 3.1 pix
The object was found in VSX 2" ASASSN-V J052653.96+353448.1
Type: SR
# Max. Min./Amp. JD0 Period
13.850 V 14.680 V 2458363.21340 348.303522200000
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:26:53.89 +35:34:49.3: 13.95 +/- 0.05 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:26:53.89 +35:34:49.3: 13.52 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.66 +/- 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 J052653.96+353448.1,2461233.9269,12.03,0.05,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 J052653.96+353448.1 20260712.4269 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4269 2461233.9269 12.70 05:02:26.25 +34:39:46.2
170.09901 -4.34939 galactic Aur Second-epoch detections are separated by 1.7" and 3.3 pix
The object was found in VSX 2" NSVS J0502262+343941
Type: SR
# Max. Min./Amp. JD0 Period
13.135 r Y 0.335 r 2458396.59760 102.970142300000
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:02:26.25 +34:39:46.2: 13.78 +/- 0.04 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:02:26.25 +34:39:46.2: 13.81 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.80 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0502262+343941,2461233.9269,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0502262+343941 20260712.4269 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4269 2461233.9269 12.29 05:36:12.72 +35:03:05.6
173.75632 1.54743 galactic Aur Second-epoch detections are separated by 0.8" and 3.4 pix
The object was found in VSX 0" NSVS J0536128+350304
Type: SR
# Max. Min./Amp. JD0 Period
12.654 r Y 0.552 r 2458522.83160 237.885503400000
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:36:12.72 +35:03:05.6: 13.62 +/- 0.05 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:36:12.72 +35:03:05.6: 13.56 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin 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 J0536128+350304,2461233.9269,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0536128+350304 20260712.4269 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4269 2461233.9269 12.44 05:33:34.46 +37:43:25.2
171.21962 2.54509 galactic Aur Second-epoch detections are separated by 3.0" and 2.9 pix
The object was found in VSX 2" NSVS J0533345+374322
Type: SR
# Max. Min./Amp. JD0 Period
13.231 r Y 0.884 r 2458469.47210 153.034937800000
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:33:34.46 +37:43:25.2: 13.98 +/- 0.05 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:33:34.46 +37:43:25.2: 13.72 +/- 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
NSVS J0533345+374322,2461233.9269,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0533345+374322 20260712.4269 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4269 2461233.9269 13.13 05:20:07.41 +37:57:30.2
169.54420 0.47104 galactic Aur Second-epoch detections are separated by 2.0" and 3.5 pix
The object was found in VSX 1" ZTF J052007.46+375731.1
Type: SR
# Max. Min./Amp. JD0 Period
13.269 r Y 0.312 r 2458338.55830 70.592721900000
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:20:07.41 +37:57:30.2: 14.06 +/- 0.06 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:20:07.41 +37:57:30.2: 14.22 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.13 +/- 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
ZTF J052007.46+375731.1,2461233.9269,13.13,0.05,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
ZTF J052007.46+375731.1 20260712.4269 13.13CV 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 12.4269 2461233.9269 11.44 05:57:27.49 +40:27:58.0
171.25651 7.92787 galactic Aur Second-epoch detections are separated by 1.2" and 3.5 pix
The object was found in VSX 1" ASASSN-V J055727.56+402758.7
Type: L
# Max. Min./Amp. JD0 Period
12.800 V 13.200 V
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:57:27.49 +40:27:58.0: 12.36 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:57:27.49 +40:27:58.0: 12.60 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.46 +/- 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 J055727.56+402758.7,2461233.9269,11.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J055727.56+402758.7 20260712.4269 11.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4269 2461233.9269 12.21 05:37:14.73 +39:16:27.9
170.29758 3.98499 galactic Aur Second-epoch detections are separated by 2.6" and 3.0 pix
The object was found in VSX 5" ZTF J053714.82+391632.4
Type: SR
# Max. Min./Amp. JD0 Period
12.356 r Y 0.671 r 2458430.07640 172.528106800000
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:37:14.73 +39:16:27.9: 13.68 +/- 0.04 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:37:14.73 +39:16:27.9: 13.66 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J053714.82+391632.4,2461233.9269,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J053714.82+391632.4 20260712.4269 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4269 2461233.9269 12.31 05:06:24.40 +39:32:46.2
166.68911 -0.76167 galactic Aur Second-epoch detections are separated by 0.7" and 3.1 pix
The object was found in VSX 2" ASASSN-V J050624.59+393247.3
Type: L
# Max. Min./Amp. JD0 Period
13.500 V 14.050 V
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:06:24.40 +39:32:46.2: 13.56 +/- 0.04 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:06:24.40 +39:32:46.2: 13.12 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.26 +/- 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 J050624.59+393247.3,2461233.9269,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J050624.59+393247.3 20260712.4269 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4269 2461233.9269 12.66 05:18:56.99 +34:57:09.1
171.87232 -1.44512 galactic Aur Second-epoch detections are separated by 0.5" and 3.3 pix
The object was found in VSX 1" OO Aur
Type: LB:
# Max. Min./Amp. JD0 Period
13.900 V 14.600 V C
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:18:56.99 +34:57:09.1: 14.18 +/- 0.09 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:18:56.99 +34:57:09.1: 13.99 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.06 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin 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
OO Aur,2461233.9269,12.66,0.05,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
OO Aur 20260712.4269 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 12.4269 2461233.9269 12.26 05:54:43.03 +41:52:12.7
169.76462 8.16313 galactic Aur Second-epoch detections are separated by 1.6" and 3.3 pix
The object was found in VSX 1" V0372 Aur
Type: LB:
# Max. Min./Amp. JD0 Period
14.300 pg 15.300 pg
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:54:43.03 +41:52:12.7: 13.34 +/- 0.03 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:54:43.03 +41:52:12.7: 13.31 +/- 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!
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
V0372 Aur,2461233.9269,12.26,0.05,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
V0372 Aur 20260712.4269 12.26CV 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 12.4269 2461233.9269 12.83 05:27:17.87 +36:39:05.8
171.42813 0.91158 galactic Aur Second-epoch detections are separated by 2.2" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J081.8242+36.6517 | 05:27:17.83 +36:39:06.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.709+/-0.036 (Very red! L if it's a dwarf)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:27:17.87 +36:39:05.8: 13.92 +/- 0.05 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:27:17.87 +36:39:05.8: 13.78 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.83 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J081.8242+36.6517,2461233.9269,12.83,0.05,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 J081.8242+36.6517 20260712.4269 12.83CV 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 12.4269 2461233.9269 12.40 05:22:09.37 +37:23:14.8
170.24260 0.47630 galactic Aur Second-epoch detections are separated by 0.5" and 3.2 pix
The object was found in VSX 0" NSVS 4385769
Type: SR
# Max. Min./Amp. JD0 Period
12.743 r Y 0.400 r 2458488.18690 180.474438800000
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:22:09.37 +37:23:14.8: 13.56 +/- 0.03 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:22:09.37 +37:23:14.8: 13.55 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 4385769,2461233.9269,12.40,0.05,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 4385769 20260712.4269 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4269 2461233.9269 12.14 05:20:45.06 +38:10:49.4
169.43253 0.69922 galactic Aur Second-epoch detections are separated by 1.8" and 3.4 pix
The object was found in VSX 1" V0487 Aur
Type: SR:
# Max. Min./Amp. JD0 Period
12.000 pg 14.100 pg 8.779630000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:20:45.06 +38:10:49.4: 13.90 +/- 0.05 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:20:45.06 +38:10:49.4: 14.05 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.97 +/- 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
V0487 Aur,2461233.9269,12.14,0.05,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
V0487 Aur 20260712.4269 12.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4269 2461233.9269 10.82 05:06:25.57 +37:34:30.5
168.26556 -1.94542 galactic Aur Second-epoch detections are separated by 0.1" and 3.1 pix
The object was found in VSX 2" ASASSN-V J050625.43+373430.8
Type: SR
# Max. Min./Amp. JD0 Period
12.320 V 12.770 V 2457291.00000 81.200000000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:06:25.57 +37:34:30.5: 11.70 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:06:25.57 +37:34:30.5: 11.77 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.74 +/- 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 J050625.43+373430.8,2461233.9269,10.82,0.05,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 J050625.43+373430.8 20260712.4269 10.82CV 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 12.4269 2461233.9269 12.01 05:47:58.87 +41:17:44.9
169.63366 6.78486 galactic Aur Second-epoch detections are separated by 2.0" and 3.1 pix
The object was found in VSX 1" ASASSN-V J054758.83+411746.1
Type: L
# Max. Min./Amp. JD0 Period
13.420 V 14.060 V
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:47:58.87 +41:17:44.9: 13.35 +/- 0.03 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:47:58.87 +41:17:44.9: 13.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.33 +/- 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 J054758.83+411746.1,2461233.9269,12.01,0.05,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
ASASSN-V J054758.83+411746.1 20260712.4269 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 12.4269 2461233.9269 12.61 05:16:59.17 +35:14:10.8
171.40874 -1.60986 galactic Aur Second-epoch detections are separated by 1.3" and 3.1 pix
The object was found in VSX 3" ASASSN-V J051659.40+351408.9
Type: SR
# Max. Min./Amp. JD0 Period
15.100 g Y 0.240 g 2459221.88800 98.190000000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:16:59.17 +35:14:10.8: 13.51 +/- 0.03 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:16:59.17 +35:14:10.8: 13.53 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.52 +/- 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 J051659.40+351408.9,2461233.9269,12.61,0.05,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
ASASSN-V J051659.40+351408.9 20260712.4269 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 12.4269 2461233.9269 12.01 05:34:46.85 +40:24:26.7
169.08436 4.19253 galactic Aur Second-epoch detections are separated by 1.7" and 3.3 pix
The object was found in VSX 1" ASASSN-V J053446.87+402427.4
Type: SR
# Max. Min./Amp. JD0 Period
13.190 V 14.110 V 2457065.80000 574.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:34:46.85 +40:24:26.7: 13.03 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:34:46.85 +40:24:26.7: 12.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.00 +/- 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 J053446.87+402427.4,2461233.9269,12.01,0.05,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
ASASSN-V J053446.87+402427.4 20260712.4269 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 12.4269 2461233.9269 12.99 05:20:36.57 +38:35:56.2
169.07296 0.91530 galactic Aur Second-epoch detections are separated by 2.5" and 2.9 pix
The object was found in VSX 1" ASASSN-V J052036.60+383555.5
Type: SR
# Max. Min./Amp. JD0 Period
15.530 g Y 0.290 g 2458903.73000 232.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:20:36.57 +38:35:56.2: 14.28 +/- 0.06 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:20:36.57 +38:35:56.2: 14.27 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.27 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J052036.60+383555.5,2461233.9269,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J052036.60+383555.5 20260712.4269 12.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461058.61200600 18.01.2026 02:41:07.318 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
First image: 2461058.61200600 18.01.2026 02:41:07.318 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
Last image: 2461233.92720451 12.07.2026 10:15:00.470 /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q1b1x1_055948_TTUQ1b1x1_572930_wIJUi5vl/fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 89
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.70
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: 9 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): 24318
Objects passed selection criteria: 24187
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: 17092
Average stars matched: 16246.2 (95.0518 %)
Memory usage VmPeak: 132748 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 06:58:33 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: 2461058.61200600 18.01.2026 02:41:07.318 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
First image: 2461058.61200600 18.01.2026 02:41:07.318 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
Last image: 2461233.92720451 12.07.2026 10:15:00.470 /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q1b1x1_055948_TTUQ1b1x1_572930_wIJUi5vl/fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 216
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.38
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: 52 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): 181147
Objects passed selection criteria: 180614
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: 129416
Average stars matched: 119086 (92.018 %)
Memory usage VmPeak: 2001896 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 07:04:54 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-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q1b1x1_055948_TTUQ1b1x1_572930_wIJUi5vl/fd_Aur-03-Q1b1x1_2026-07-12_05-14-16_20.00sec_-0.00C_LIGHTs_0430.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q1b1x1_055948_TTUQ1b1x1_572930_wIJUi5vl/fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431.fits
SExtractor catalog cache: saved Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.cat to cache
SExtractor catalog cache: saved Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.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-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q1b1x1_055948_TTUQ1b1x1_572930_wIJUi5vl/fd_Aur-03-Q1b1x1_2026-07-12_05-14-16_20.00sec_-0.00C_LIGHTs_0430.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q1b1x1_055948_TTUQ1b1x1_572930_wIJUi5vl/fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431.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: 2461233.92668983
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits exists and is non-empty
Saving wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits to local_wcs_cache/
'wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits' -> 'local_wcs_cache/wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits'
wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits exists and is non-empty
Saving wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits to local_wcs_cache/
'wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits' -> 'local_wcs_cache/wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits'
wcs_fd_Aur-03-Q1b1x1_2026-07-12_05-14-16_20.00sec_-0.00C_LIGHTs_0430.fits exists and is non-empty
Saving wcs_fd_Aur-03-Q1b1x1_2026-07-12_05-14-16_20.00sec_-0.00C_LIGHTs_0430.fits to local_wcs_cache/
'wcs_fd_Aur-03-Q1b1x1_2026-07-12_05-14-16_20.00sec_-0.00C_LIGHTs_0430.fits' -> 'local_wcs_cache/wcs_fd_Aur-03-Q1b1x1_2026-07-12_05-14-16_20.00sec_-0.00C_LIGHTs_0430.fits'
wcs_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431.fits exists and is non-empty
Saving wcs_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431.fits to local_wcs_cache/
'wcs_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431.fits' -> 'local_wcs_cache/wcs_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits (1st reference image)
verification OK: wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
Image size: 941.6'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: 05:27:17.024 +37:59:58.79 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-03-Q1b1x1_2026-07-12_05-14-16_20.00sec_-0.00C_LIGHTs_0430.fits (1st new image)
verification OK: wcs_fd_Aur-03-Q1b1x1_2026-07-12_05-14-16_20.00sec_-0.00C_LIGHTs_0430.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: 05:27:22.122 +38:00:57.51 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:27:17.024 +37:59:58.79
Second-epoch image center 05:27:22.122 +38:00:57.51
Angular distance between the image centers 0.0234 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431.fits (2nd new image)
verification OK: wcs_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431.fits
Image size: 946.6'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: 05:27:21.009 +38:00:43.20 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:27:17.024 +37:59:58.79
Second-epoch image center 05:27:21.009 +38:00:43.20
Angular distance between the image centers 0.0180 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 05:27:22.122 +38:00:57.51
Second-epoch second image center 05:27:21.009 +38:00:43.20
Angular distance between the image centers 0.00540 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-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits &> /tmp/tmp.fuj5cxFCnh
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits &> /tmp/tmp.fyWXJazb6O
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q1b1x1_055948_TTUQ1b1x1_572930_wIJUi5vl/fd_Aur-03-Q1b1x1_2026-07-12_05-14-16_20.00sec_-0.00C_LIGHTs_0430.fits &> /tmp/tmp.BUlqhEIRZY
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q1b1x1_055948_TTUQ1b1x1_572930_wIJUi5vl/fd_Aur-03-Q1b1x1_2026-07-12_05-14-16_20.00sec_-0.00C_LIGHTs_0430.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q1b1x1_055948_TTUQ1b1x1_572930_wIJUi5vl/fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431.fits &> /tmp/tmp.EdIWmzB00Q
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q1b1x1_055948_TTUQ1b1x1_572930_wIJUi5vl/fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.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-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits and wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.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-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits and wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat
Found non-empty wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits and wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat
The reference image (wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits) and catalog (wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat) found
'wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat' -> 'wcsmag.cat'
Read 27843 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 70.8766 to 92.1250 deg, Dec +31.9889 to +43.3926 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 70.8766 to 92.1250 deg, Dec 31.9889 to 43.3926 deg
Loaded 16031 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): 11098 out of 12445 total matches.
Matched with Tycho-2 12445 out of 27843 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.926900
a=0.000000 b=1.000000 c=22.926900
From vast_summary.log: estimated ref. image limiting mag.: -7.70
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.23
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.23
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 27843 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 70.8766 to 92.1250 deg, Dec +31.9889 to +43.3926 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 70.8766 to 92.1250 deg, Dec 31.9889 to 43.3926 deg
Loaded 16031 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): 11098 out of 12445 total matches.
Matched with Tycho-2 12445 out of 27843 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits:
Forced-photometry filter: calibrated wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits -> calib.txt_param_ref_wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits (aperture=6.2)
Read 27116 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 71.3508 to 92.6935 deg, Dec +32.1410 to +43.3194 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 71.3508 to 92.6935 deg, Dec 32.1410 to 43.3194 deg
Loaded 16021 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): 10961 out of 12446 total matches.
Matched with Tycho-2 12446 out of 27116 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits:
Forced-photometry filter: calibrated wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits -> calib.txt_param_ref_wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits (aperture=6.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 82 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
2.1 pix Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
2.9 pix fd_Aur-03-Q1b1x1_2026-07-12_05-14-16_20.00sec_-0.00C_LIGHTs_0430.fits
2.9 pix fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431.fits
2.2 pix wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
2.1 pix wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
Limiting magnitude estimates:
15.2 mag. Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
15.2 mag. Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
13.2 mag. fd_Aur-03-Q1b1x1_2026-07-12_05-14-16_20.00sec_-0.00C_LIGHTs_0430.fits
13.2 mag. fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431.fits
All-image limiting magnitude estimate: 13.2 (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.fuj5cxFCnh (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-03-Q1b1x1_055948_TTUQ1b1x1_572930_wIJUi5vl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.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-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits' -> 'wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
WCS_IMAGE_NAME=wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
WCS-calibrated image found: wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
Checking if the catalog wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat corresponding to the image wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits alredy exist and is non-empty...
Catalog wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat corresponding to the image wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
WCS catalog name: wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.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=2982, bad_region=0, passed=27843
Got 27843 stars (including 24835 good ones) from the SExtractor catalog wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat
util/solve_plate_with_UCAC5 got 27843 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 609 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 916 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 26352 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 609 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 26354 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 26354 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 952 stars left (next iteration limit 1047)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits N_match=952 sigma_overall_arcsec=0.445 sigma_q1_arcsec=0.538 sigma_q2_arcsec=0.345 sigma_q3_arcsec=0.438 sigma_q4_arcsec=0.338 n_q1=171 n_q2=289 n_q3=232 n_q4=260 worst_quadrant_to_overall_ratio=1.208
The image catalog is written to wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits -region wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.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.fyWXJazb6O (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-03-Q1b1x1_055948_TTUQ1b1x1_572930_wIJUi5vl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.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-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits' -> 'wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
WCS_IMAGE_NAME=wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
WCS-calibrated image found: wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
Checking if the catalog wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat corresponding to the image wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits alredy exist and is non-empty...
Catalog wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat corresponding to the image wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
WCS catalog name: wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.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=3147, bad_region=0, passed=27116
Got 27116 stars (including 23937 good ones) from the SExtractor catalog wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat
util/solve_plate_with_UCAC5 got 27116 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 610 to 668 (Dec 32.1 to 43.3)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 910 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 25839 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
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 610 to 668 (Dec 32.1 to 43.3)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 25837 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 25836 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 943 stars left (next iteration limit 1037)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits N_match=943 sigma_overall_arcsec=0.591 sigma_q1_arcsec=0.674 sigma_q2_arcsec=0.543 sigma_q3_arcsec=0.480 sigma_q4_arcsec=0.620 n_q1=207 n_q2=291 n_q3=244 n_q4=201 worst_quadrant_to_overall_ratio=1.141
The image catalog is written to wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits -region wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.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.BUlqhEIRZY (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-03-Q1b1x1_055948_TTUQ1b1x1_572930_wIJUi5vl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q1b1x1_055948_TTUQ1b1x1_572930_wIJUi5vl/fd_Aur-03-Q1b1x1_2026-07-12_05-14-16_20.00sec_-0.00C_LIGHTs_0430.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q1b1x1_055948_TTUQ1b1x1_572930_wIJUi5vl/fd_Aur-03-Q1b1x1_2026-07-12_05-14-16_20.00sec_-0.00C_LIGHTs_0430.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q1b1x1_055948_TTUQ1b1x1_572930_wIJUi5vl/fd_Aur-03-Q1b1x1_2026-07-12_05-14-16_20.00sec_-0.00C_LIGHTs_0430.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q1b1x1_055948_TTUQ1b1x1_572930_wIJUi5vl/fd_Aur-03-Q1b1x1_2026-07-12_05-14-16_20.00sec_-0.00C_LIGHTs_0430.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q1b1x1_055948_TTUQ1b1x1_572930_wIJUi5vl/fd_Aur-03-Q1b1x1_2026-07-12_05-14-16_20.00sec_-0.00C_LIGHTs_0430.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-03-Q1b1x1_055948_TTUQ1b1x1_572930_wIJUi5vl/fd_Aur-03-Q1b1x1_2026-07-12_05-14-16_20.00sec_-0.00C_LIGHTs_0430.fits
WCS_IMAGE_NAME=wcs_fd_Aur-03-Q1b1x1_2026-07-12_05-14-16_20.00sec_-0.00C_LIGHTs_0430.fits
WCS-calibrated image found: wcs_fd_Aur-03-Q1b1x1_2026-07-12_05-14-16_20.00sec_-0.00C_LIGHTs_0430.fits
Checking if the catalog wcs_fd_Aur-03-Q1b1x1_2026-07-12_05-14-16_20.00sec_-0.00C_LIGHTs_0430.fits.wcscat corresponding to the image wcs_fd_Aur-03-Q1b1x1_2026-07-12_05-14-16_20.00sec_-0.00C_LIGHTs_0430.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-03-Q1b1x1_2026-07-12_05-14-16_20.00sec_-0.00C_LIGHTs_0430.fits.wcscat corresponding to the image wcs_fd_Aur-03-Q1b1x1_2026-07-12_05-14-16_20.00sec_-0.00C_LIGHTs_0430.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-03-Q1b1x1_2026-07-12_05-14-16_20.00sec_-0.00C_LIGHTs_0430.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-03-Q1b1x1_055948_TTUQ1b1x1_572930_wIJUi5vl/fd_Aur-03-Q1b1x1_2026-07-12_05-14-16_20.00sec_-0.00C_LIGHTs_0430.fits
WCS catalog name: wcs_fd_Aur-03-Q1b1x1_2026-07-12_05-14-16_20.00sec_-0.00C_LIGHTs_0430.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=9, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=271, bad_region=0, passed=6890
Got 6890 stars (including 6612 good ones) from the SExtractor catalog wcs_fd_Aur-03-Q1b1x1_2026-07-12_05-14-16_20.00sec_-0.00C_LIGHTs_0430.fits.wcscat
util/solve_plate_with_UCAC5 got 6890 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 610 to 669 (Dec 32.1 to 43.4)
Done reading UCAC5 zone files...
Matched 937 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(), 898 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 6545 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 610 to 669 (Dec 32.1 to 43.4)
Done reading UCAC5 zone files...
Matched 937 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(), 6547 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 6547 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
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-03-Q1b1x1_2026-07-12_05-14-16_20.00sec_-0.00C_LIGHTs_0430.fits N_match=935 sigma_overall_arcsec=0.597 sigma_q1_arcsec=0.582 sigma_q2_arcsec=0.874 sigma_q3_arcsec=0.493 sigma_q4_arcsec=0.743 n_q1=206 n_q2=143 n_q3=386 n_q4=200 worst_quadrant_to_overall_ratio=1.463
The image catalog is written to wcs_fd_Aur-03-Q1b1x1_2026-07-12_05-14-16_20.00sec_-0.00C_LIGHTs_0430.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-03-Q1b1x1_2026-07-12_05-14-16_20.00sec_-0.00C_LIGHTs_0430.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q1b1x1_055948_TTUQ1b1x1_572930_wIJUi5vl/fd_Aur-03-Q1b1x1_2026-07-12_05-14-16_20.00sec_-0.00C_LIGHTs_0430.fits -region wcs_fd_Aur-03-Q1b1x1_2026-07-12_05-14-16_20.00sec_-0.00C_LIGHTs_0430.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-03-Q1b1x1_2026-07-12_05-14-16_20.00sec_-0.00C_LIGHTs_0430.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.EdIWmzB00Q (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-03-Q1b1x1_055948_TTUQ1b1x1_572930_wIJUi5vl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q1b1x1_055948_TTUQ1b1x1_572930_wIJUi5vl/fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q1b1x1_055948_TTUQ1b1x1_572930_wIJUi5vl/fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q1b1x1_055948_TTUQ1b1x1_572930_wIJUi5vl/fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q1b1x1_055948_TTUQ1b1x1_572930_wIJUi5vl/fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q1b1x1_055948_TTUQ1b1x1_572930_wIJUi5vl/fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431.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-03-Q1b1x1_055948_TTUQ1b1x1_572930_wIJUi5vl/fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431.fits
WCS_IMAGE_NAME=wcs_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431.fits
WCS-calibrated image found: wcs_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431.fits
Checking if the catalog wcs_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431.fits.wcscat corresponding to the image wcs_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431.fits.wcscat corresponding to the image wcs_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431.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-03-Q1b1x1_055948_TTUQ1b1x1_572930_wIJUi5vl/fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431.fits
WCS catalog name: wcs_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431.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=1, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=317, bad_region=0, passed=6940
Got 6940 stars (including 6618 good ones) from the SExtractor catalog wcs_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431.fits.wcscat
util/solve_plate_with_UCAC5 got 6940 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 946.6'
Seting catalog search parameters based on the expected field of view 946.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013147 (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 0.010518 (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 610 to 669 (Dec 32.0 to 43.4)
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(), 898 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 6580 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 669 (Dec 32.0 to 43.4)
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(), 6579 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 6579 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-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431.fits N_match=933 sigma_overall_arcsec=0.614 sigma_q1_arcsec=0.553 sigma_q2_arcsec=0.836 sigma_q3_arcsec=0.490 sigma_q4_arcsec=0.672 n_q1=206 n_q2=145 n_q3=378 n_q4=204 worst_quadrant_to_overall_ratio=1.363
The image catalog is written to wcs_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q1b1x1_055948_TTUQ1b1x1_572930_wIJUi5vl/fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431.fits -region wcs_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431.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-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits sigma_overall=0.445 worst_q_ratio=1.208
ref2=Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits sigma_overall=0.591 worst_q_ratio=1.141
new1=fd_Aur-03-Q1b1x1_2026-07-12_05-14-16_20.00sec_-0.00C_LIGHTs_0430.fits sigma_overall=0.597 worst_q_ratio=1.463
new2=fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431.fits sigma_overall=0.614 worst_q_ratio=1.363
reference average sigma_overall=0.518 worst_q_ratio=1.1745
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049_astrometric_residuals.png (952 matched stars from wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.38 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054_astrometric_residuals.png (943 matched stars from wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.52 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aur-03-Q1b1x1_2026-07-12_05-14-16_20.00sec_-0.00C_LIGHTs_0430_astrometric_residuals.png (935 matched stars from wcs_fd_Aur-03-Q1b1x1_2026-07-12_05-14-16_20.00sec_-0.00C_LIGHTs_0430.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.51 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431_astrometric_residuals.png (933 matched stars from wcs_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.55 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aur-03-Q1b1x1_2026-07-12_05-14-16_20.00sec_-0.00C_LIGHTs_0430.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-03-Q1b1x1_2026-07-12_05-14-16_20.00sec_-0.00C_LIGHTs_0430.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q1b1x1_055948_TTUQ1b1x1_572930_wIJUi5vl/wcs_fd_Aur-03-Q1b1x1_2026-07-12_05-14-16_20.00sec_-0.00C_LIGHTs_0430.fits'
Saving fully-calibrated image wcs_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q1b1x1_055948_TTUQ1b1x1_572930_wIJUi5vl/wcs_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431.fits'
Preparing the HTML report for the field Aur-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:58:08.41 +34:07:07.1: 99.00 +/- 99.00 saturated
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:03:34.71 +35:49:55.7: 99.00 +/- 99.00 saturated
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:59:31.01 +34:30:11.7: 99.00 +/- 99.00 saturated
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:53:02.97 +33:09:26.2: 9.28 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:06:05.90 +37:03:17.8: 99.00 +/- 99.00 saturated
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:02:04.73 +35:37:45.3: 9.26 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:03:47.75 +36:25:04.4: 9.17 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:04:44.53 +35:25:20.1: 9.08 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:58:08.41 +34:07:07.1: 99.00 +/- 99.00 saturated
Forced photometry filter REJECTED candidate at 05:58:08.41 +34:07:07.1: 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-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:04:10.90 +36:02:59.4: 9.23 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:03:34.71 +35:49:55.7: 99.00 +/- 99.00 saturated
Forced photometry filter REJECTED candidate at 06:03:34.71 +35:49:55.7: 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-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:02:04.73 +35:37:45.3: 99.00 +/- 99.00 saturated
Forced photometry filter REJECTED candidate at 06:02:04.73 +35:37:45.3: 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-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:04:44.53 +35:25:20.1: 99.00 +/- 99.00 saturated
Forced photometry filter REJECTED candidate at 06:04:44.53 +35:25:20.1: 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-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:06:05.90 +37:03:17.8: 99.00 +/- 99.00 saturated
Forced photometry filter REJECTED candidate at 06:06:05.90 +37:03:17.8: 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-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:53:02.97 +33:09:26.2: 99.00 +/- 99.00 saturated
Forced photometry filter REJECTED candidate at 05:53:02.97 +33:09:26.2: 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-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:59:31.01 +34:30:11.7: 99.00 +/- 99.00 saturated
Forced photometry filter REJECTED candidate at 05:59:31.01 +34:30:11.7: 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-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:03:47.75 +36:25:04.4: 99.00 +/- 99.00 saturated
Forced photometry filter REJECTED candidate at 06:03:47.75 +36:25:04.4: 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-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:00:17.81 +34:09:40.5: 9.42 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:04:10.90 +36:02:59.4: 99.00 +/- 99.00 saturated
Forced photometry filter REJECTED candidate at 06:04:10.90 +36:02:59.4: 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-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:00:17.81 +34:09:40.5: 99.00 +/- 99.00 saturated
Forced photometry filter REJECTED candidate at 06:00:17.81 +34:09:40.5: 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-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:57:44.53 +34:38:47.2: 9.50 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:01:12.11 +35:16:21.3: 9.14 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:01:35.13 +35:05:53.0: 9.39 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:02:22.37 +34:47:26.6: 9.34 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:58:19.04 +34:18:36.2: 9.63 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:54:47.44 +33:04:43.5: 9.20 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:01:22.96 +35:35:38.8: 9.70 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:55:53.27 +34:21:27.9: 9.52 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:57:44.53 +34:38:47.2: 99.00 +/- 99.00 saturated
Forced photometry filter REJECTED candidate at 05:57:44.53 +34:38:47.2: 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-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:57:53.02 +33:49:42.5: 9.47 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:01:12.11 +35:16:21.3: 9.22 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.18 +/- 0.00
Forced photometry filter REJECTED candidate at 06:01:12.11 +35:16:21.3: ref_mag=9.18 +/- 0.00 new_mean_mag=9.7490 delta=-0.56 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:02:22.37 +34:47:26.6: 9.37 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:54:47.44 +33:04:43.5: 99.00 +/- 99.00 saturated
Forced photometry filter REJECTED candidate at 05:54:47.44 +33:04:43.5: 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-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:01:35.13 +35:05:53.0: 99.00 +/- 99.00 saturated
Forced photometry filter REJECTED candidate at 06:01:35.13 +35:05:53.0: 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-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:01:22.96 +35:35:38.8: 9.74 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:58:19.04 +34:18:36.2: 9.69 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.35 +/- 0.00
Forced photometry filter REJECTED candidate at 06:02:22.37 +34:47:26.6: ref_mag=9.35 +/- 0.00 new_mean_mag=9.7724 delta=-0.42 (need > 0.90)
Forced photometry reference-image weighted average: 9.72 +/- 0.00
Forced photometry reference-image weighted average: 9.66 +/- 0.00
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:03:21.40 +36:11:37.0: 9.66 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 06:01:22.96 +35:35:38.8: ref_mag=9.72 +/- 0.00 new_mean_mag=9.9196 delta=-0.20 (need > 0.90)
Forced photometry filter REJECTED candidate at 05:58:19.04 +34:18:36.2: ref_mag=9.66 +/- 0.00 new_mean_mag=9.8992 delta=-0.24 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:55:53.27 +34:21:27.9: 9.54 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.53 +/- 0.00
Forced photometry filter REJECTED candidate at 05:55:53.27 +34:21:27.9: ref_mag=9.53 +/- 0.00 new_mean_mag=9.9617 delta=-0.43 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:57:53.02 +33:49:42.5: 99.00 +/- 99.00 saturated
Forced photometry filter REJECTED candidate at 05:57:53.02 +33:49:42.5: 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-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:03:21.40 +36:11:37.0: 9.71 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.69 +/- 0.00
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:04:25.75 +35:57:11.4: 9.70 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 06:03:21.40 +36:11:37.0: ref_mag=9.69 +/- 0.00 new_mean_mag=9.9555 delta=-0.27 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:54:50.19 +33:30:47.0: 9.75 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:01:39.52 +33:46:08.4: 9.25 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:54:17.75 +33:10:00.6: 9.67 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:05:23.55 +36:21:50.2: 9.41 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:57:54.94 +34:54:41.0: 10.20 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:01:54.55 +35:44:32.4: 9.58 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:04:25.75 +35:57:11.4: 9.78 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.74 +/- 0.00
Forced photometry filter REJECTED candidate at 06:04:25.75 +35:57:11.4: ref_mag=9.74 +/- 0.00 new_mean_mag=10.0096 delta=-0.27 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:56:06.15 +32:55:38.0: 9.43 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:02:52.66 +34:22:31.5: 10.45 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:54:50.19 +33:30:47.0: 9.80 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.78 +/- 0.00
Forced photometry filter REJECTED candidate at 05:54:50.19 +33:30:47.0: ref_mag=9.78 +/- 0.00 new_mean_mag=10.0479 delta=-0.27 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:01:39.52 +33:46:08.4: 99.00 +/- 99.00 saturated
Forced photometry filter REJECTED candidate at 06:01:39.52 +33:46:08.4: 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-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:05:23.55 +36:21:50.2: 9.48 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:54:17.75 +33:10:00.6: 9.70 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:01:54.55 +35:44:32.4: 9.66 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:57:54.94 +34:54:41.0: 10.22 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.45 +/- 0.00
Forced photometry reference-image weighted average: 9.69 +/- 0.00
Forced photometry filter REJECTED candidate at 06:05:23.55 +36:21:50.2: ref_mag=9.45 +/- 0.00 new_mean_mag=10.0563 delta=-0.61 (need > 0.90)
Forced photometry filter REJECTED candidate at 05:54:17.75 +33:10:00.6: ref_mag=9.69 +/- 0.00 new_mean_mag=10.0780 delta=-0.39 (need > 0.90)
Forced photometry reference-image weighted average: 9.61 +/- 0.00
Forced photometry reference-image weighted average: 10.21 +/- 0.00
Forced photometry filter REJECTED candidate at 05:57:54.94 +34:54:41.0: ref_mag=10.21 +/- 0.00 new_mean_mag=10.0828 delta=0.13 (need > 0.90)
Forced photometry filter REJECTED candidate at 06:01:54.55 +35:44:32.4: ref_mag=9.61 +/- 0.00 new_mean_mag=10.0951 delta=-0.48 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:57:44.59 +34:55:16.9: 9.56 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:56:06.15 +32:55:38.0: 99.00 +/- 99.00 saturated
Forced photometry filter REJECTED candidate at 05:56:06.15 +32:55:38.0: 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-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:02:52.66 +34:22:31.5: 10.53 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.49 +/- 0.00
Forced photometry filter REJECTED candidate at 06:02:52.66 +34:22:31.5: ref_mag=10.49 +/- 0.00 new_mean_mag=10.1195 delta=0.37 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:57:44.59 +34:55:16.9: 9.59 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:00:46.80 +34:15:33.3: 9.64 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.57 +/- 0.00
Forced photometry filter REJECTED candidate at 05:57:44.59 +34:55:16.9: ref_mag=9.57 +/- 0.00 new_mean_mag=10.1739 delta=-0.60 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:57:31.43 +33:53:25.9: 9.86 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:56:23.67 +33:17:38.4: 10.30 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:59:29.57 +33:00:10.3: 9.76 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:56:13.55 +33:52:39.7: 10.33 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:01:24.29 +33:51:16.4: 10.53 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:55:13.18 +34:02:55.9: 10.74 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:00:46.80 +34:15:33.3: 9.70 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.67 +/- 0.00
Forced photometry filter REJECTED candidate at 06:00:46.80 +34:15:33.3: ref_mag=9.67 +/- 0.00 new_mean_mag=10.0693 delta=-0.39 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:57:11.77 +33:42:58.4: 9.76 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:00:09.27 +33:54:27.0: 9.43 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:57:31.43 +33:53:25.9: 9.91 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.89 +/- 0.00
Forced photometry filter REJECTED candidate at 05:57:31.43 +33:53:25.9: ref_mag=9.89 +/- 0.00 new_mean_mag=10.1762 delta=-0.29 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:56:23.67 +33:17:38.4: 10.26 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.28 +/- 0.00
Forced photometry filter REJECTED candidate at 05:56:23.67 +33:17:38.4: ref_mag=10.28 +/- 0.00 new_mean_mag=10.0380 delta=0.24 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:59:29.57 +33:00:10.3: 9.86 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:56:13.55 +33:52:39.7: 10.39 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.81 +/- 0.00
Forced photometry reference-image weighted average: 10.36 +/- 0.00
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:01:24.29 +33:51:16.4: 10.50 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 05:59:29.57 +33:00:10.3: ref_mag=9.81 +/- 0.00 new_mean_mag=10.0565 delta=-0.24 (need > 0.90)
Forced photometry filter REJECTED candidate at 05:56:13.55 +33:52:39.7: ref_mag=10.36 +/- 0.00 new_mean_mag=10.1369 delta=0.22 (need > 0.90)
Forced photometry reference-image weighted average: 10.51 +/- 0.00
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:55:13.18 +34:02:55.9: 10.68 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 06:01:24.29 +33:51:16.4: ref_mag=10.51 +/- 0.00 new_mean_mag=10.1321 delta=0.38 (need > 0.90)
Forced photometry reference-image weighted average: 10.71 +/- 0.00
Forced photometry filter REJECTED candidate at 05:55:13.18 +34:02:55.9: ref_mag=10.71 +/- 0.00 new_mean_mag=10.2745 delta=0.43 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:02:00.57 +35:51:56.7: 10.07 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:57:11.77 +33:42:58.4: 9.82 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.79 +/- 0.00
Forced photometry filter REJECTED candidate at 05:57:11.77 +33:42:58.4: ref_mag=9.79 +/- 0.00 new_mean_mag=10.2392 delta=-0.45 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:00:09.27 +33:54:27.0: 99.00 +/- 99.00 saturated
Forced photometry filter REJECTED candidate at 06:00:09.27 +33:54:27.0: 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-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:02:51.07 +33:16:42.9: 9.75 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:02:00.57 +35:51:56.7: 10.13 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.10 +/- 0.00
Forced photometry filter REJECTED candidate at 06:02:00.57 +35:51:56.7: ref_mag=10.10 +/- 0.00 new_mean_mag=10.3157 delta=-0.21 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:00:54.34 +34:09:46.6: 10.39 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:00:40.39 +34:02:43.5: 9.63 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:47:32.85 +39:27:53.1: 11.55 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:20:55.63 +35:05:21.4: 11.36 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:02:51.07 +33:16:42.9: 9.84 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.79 +/- 0.00
Forced photometry filter REJECTED candidate at 06:02:51.07 +33:16:42.9: ref_mag=9.79 +/- 0.00 new_mean_mag=10.0728 delta=-0.28 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:00:54.34 +34:09:46.6: 10.46 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.43 +/- 0.00
Forced photometry filter REJECTED candidate at 06:00:54.34 +34:09:46.6: ref_mag=10.43 +/- 0.00 new_mean_mag=10.3044 delta=0.12 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:41:55.89 +38:56:00.6: 11.34 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:00:40.39 +34:02:43.5: 9.70 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.66 +/- 0.00
Forced photometry filter REJECTED candidate at 06:00:40.39 +34:02:43.5: ref_mag=9.66 +/- 0.00 new_mean_mag=10.3152 delta=-0.65 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:18:19.01 +35:14:59.8: 12.48 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:10:20.38 +39:49:22.9: 11.92 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:47:32.85 +39:27:53.1: 11.58 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.57 +/- 0.01
Forced photometry filter KEPT candidate at 05:47:32.85 +39:27:53.1: ref_mag=11.57 +/- 0.01 new_mean_mag=10.6009 delta=0.97 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:20:55.63 +35:05:21.4: 10.95 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.09 +/- 0.00
Forced photometry filter KEPT candidate at 05:20:55.63 +35:05:21.4: ref_mag=11.09 +/- 0.00 new_mean_mag=9.9086 delta=1.18 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:57:29.31 +41:11:02.9: 11.29 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:21:01.14 +38:28:04.6: 12.08 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:41:55.89 +38:56:00.6: 12.08 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.52 +/- 0.01
Forced photometry filter KEPT candidate at 05:41:55.89 +38:56:00.6: ref_mag=11.52 +/- 0.01 new_mean_mag=9.9814 delta=1.53 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:18:19.01 +35:14:59.8: 12.22 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.32 +/- 0.01
Forced photometry filter KEPT candidate at 05:18:19.01 +35:14:59.8: ref_mag=12.32 +/- 0.01 new_mean_mag=10.3358 delta=1.99 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:10:20.38 +39:49:22.9: 12.01 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.96 +/- 0.01
Forced photometry filter KEPT candidate at 05:10:20.38 +39:49:22.9: ref_mag=11.96 +/- 0.01 new_mean_mag=10.9240 delta=1.04 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:57:29.31 +41:11:02.9: 11.38 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.33 +/- 0.00
Forced photometry filter KEPT candidate at 05:57:29.31 +41:11:02.9: ref_mag=11.33 +/- 0.00 new_mean_mag=10.3598 delta=0.97 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:21:01.14 +38:28:04.6: 11.97 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.02 +/- 0.01
Forced photometry filter KEPT candidate at 05:21:01.14 +38:28:04.6: ref_mag=12.02 +/- 0.01 new_mean_mag=10.7855 delta=1.24 (need > 0.90)
Adding exclusion_list_local.txt__out06373.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06908.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13951.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14476.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15871.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17842.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20790.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 10s
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: 4s
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Considering the candidate 33138_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33138_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 06:00:25.07 +34:30:23.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 33143_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33143_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 06:00:14.95 +33:08:07.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 33146_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33146_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 06:04:03.23 +34:22:28.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 33147_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33147_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:57:39.59 +33:15:36.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 33148_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33148_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 06:00:28.34 +35:18:44.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 33150_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33150_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 06:03:34.38 +33:53:05.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 33152_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33152_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:57:59.73 +34:01:32.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 33157_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33157_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:26:54.62 +36:54:10.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33166_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33166_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 06:01:05.01 +35:15:31.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 33174_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33174_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:56:23.66 +33:13:08.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 33176_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33176_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:57:13.35 +32:54:51.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 33177_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33177_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:57:24.94 +33:08:04.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 33178_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33178_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 33182_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33182_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:07:56.98 +37:48:57.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33184_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33184_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 06:02:01.16 +33:16:28.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 33187_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33187_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:53:40.01 +33:44:11.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 33188_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33188_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 06:02:18.46 +35:20:06.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 33190_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33190_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 06:01:37.93 +34:50:24.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33192_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33192_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 06:01:28.82 +35:12:27.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 33197_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33197_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 06:03:40.55 +35:08:50.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 33202_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33202_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 33206_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33206_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 33209_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33209_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 33210_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33210_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:50:25.42 +32:52:46.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 33212_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33212_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 06:04:06.41 +34:40:59.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 33213_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33213_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 33215_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33215_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 33218_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33218_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 33219_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33219_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 33225_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33225_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:57:23.19 +34:09:10.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 33226_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33226_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 33228_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33228_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 33229_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33229_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 33230_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33230_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 33231_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33231_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 33235_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33235_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 33237_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33237_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:59:32.69 +32:53:06.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 33244_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33244_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 33249_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33249_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 33250_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33250_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 33255_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33255_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 33257_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33257_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 33264_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33264_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 33265_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33265_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 33267_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33267_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 33268_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33268_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 33273_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33273_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 33274_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33274_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 33275_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33275_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 33276_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33276_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 33277_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33277_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 33278_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33278_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 33280_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33280_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 33284_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33284_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 33285_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33285_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 33286_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33286_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 33287_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33287_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 33293_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33293_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 33295_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33295_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 33307_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33307_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 33308_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33308_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 33310_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33310_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 33311_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33311_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 33313_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33313_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 33326_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33326_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 33328_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33328_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 15871_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
Preparing report for the candidate 15871_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
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Considering the candidate 03860_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 03860_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:27:07.48 +34:08:59.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 16474_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 16474_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 06:01:07.19 +39:40:12.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 06373_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
Preparing report for the candidate 06373_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
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Considering the candidate 05639_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 05639_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:13:20.77 +34:37:04.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 14476_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
Preparing report for the candidate 14476_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
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Considering the candidate 06908_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
Preparing report for the candidate 06908_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
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Considering the candidate 17842_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
Preparing report for the candidate 17842_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
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Considering the candidate 20790_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
Preparing report for the candidate 20790_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
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Considering the candidate 13951_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
Preparing report for the candidate 13951_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
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Considering the candidate 04473_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 04473_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:27:38.85 +34:28:35.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 14902_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 14902_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:49:10.10 +39:10:48.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 01895_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 01895_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:18:10.73 +33:22:15.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 10519_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 10519_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:51:02.24 +37:18:18.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 14800_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 14800_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:51:29.01 +39:08:52.5 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 10151_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 10151_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 245414_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 245414_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 245418_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 245418_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:04:18.50 +39:36:34.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 245420_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 245420_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 245429_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 245429_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 04:58:15.05 +38:10:57.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 245432_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 245432_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 245438_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 245438_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:34:07.65 +39:56:42.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 245439_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 245439_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 245443_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 245443_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 245444_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 245444_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 245445_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 245445_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:29:04.18 +32:58:51.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 245446_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 245446_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:33:59.23 +41:59:14.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 245448_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 245448_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:17:52.88 +42:59:43.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 245450_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 245450_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:04:36.64 +39:49:46.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 245695_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 245695_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 245826_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 245826_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:19:15.59 +40:07:51.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 245872_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 245872_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 245925_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 245925_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 246030_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 246030_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 04:56:58.16 +33:06:02.0 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 246076_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 246076_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:13:19.97 +38:30:50.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 246119_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 246119_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:24:43.01 +37:25:05.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 246149_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 246149_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:00:16.27 +39:38:29.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 246154_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 246154_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 04:52:57.82 +42:34:49.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 246163_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 246163_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 246324_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 246324_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:10:27.41 +37:19:04.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 246466_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 246466_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:18:29.91 +42:47:09.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 246489_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 246489_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:50:58.00 +37:20:53.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 246492_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 246492_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 04:56:57.10 +33:07:03.3 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 246575_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
Preparing report for the candidate 246575_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
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Considering the candidate 246621_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 246621_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246635_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 246635_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:24:47.08 +37:21:51.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246663_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 246663_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:18:18.11 +33:47:33.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 246693_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 246693_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:27:41.43 +34:26:45.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 246700_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 246700_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 246717_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 246717_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:19:01.53 +41:06:59.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246759_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 246759_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
Rejecting candidate due to large distance (18.4") between the two second-epoch detections
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Considering the candidate 246835_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 246835_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:49:06.69 +39:13:06.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 246887_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 246887_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:17:19.76 +39:28:44.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246950_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 246950_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246963_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 246963_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:13:19.34 +38:28:10.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247011_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 247011_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:00:11.11 +39:24:17.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247027_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 247027_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:01:49.02 +42:09:55.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247060_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 247060_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 247086_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 247086_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 04:51:41.77 +42:03:19.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247139_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 247139_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247148_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 247148_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:30:54.29 +39:49:17.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247333_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 247333_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:13:46.47 +41:12:09.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247376_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 247376_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 04:51:55.95 +42:03:20.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247408_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 247408_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247484_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 247484_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:18:32.25 +40:27:40.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 247506_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 247506_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:02:27.89 +42:08:54.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247515_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 247515_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
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Considering the candidate 247551_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 247551_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:24:49.88 +37:22:47.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247557_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 247557_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247584_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 247584_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 04:49:41.71 +40:44:18.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247602_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 247602_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 04:58:54.60 +41:03:07.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247621_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 247621_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
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Considering the candidate 247630_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 247630_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
Rejecting candidate due to large distance (18.3") between the two second-epoch detections
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Considering the candidate 247632_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 247632_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247635_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 247635_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
Rejecting candidate due to large distance (19.4") between the two second-epoch detections
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Considering the candidate 247642_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 247642_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247647_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 247647_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 04:56:07.87 +35:10:59.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247648_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 247648_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:00:37.56 +40:15:22.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247690_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 247690_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247692_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 247692_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247695_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 247695_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:30:33.80 +33:00:24.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 2.842 3448981196797635968 082.64079642648 +33.00596120215 13.2711 11.4167 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.842#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 247732_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 247732_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:00:18.05 +39:25:02.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 247754_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 247754_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:06:33.92 +35:29:45.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247764_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 247764_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:09:36.32 +38:39:30.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247765_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 247765_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:17:58.04 +35:10:55.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247771_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 247771_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:45:47.07 +40:29:16.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 247780_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 247780_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:00:09.28 +39:38:54.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247819_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 247819_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:14:45.08 +39:31:19.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247829_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 247829_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 247889_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 247889_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
Rejecting candidate due to large distance (46.5") between the two second-epoch detections
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Considering the candidate 247922_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 247922_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:06:49.57 +42:15:32.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247936_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 247936_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 247990_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 247990_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
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Considering the candidate 248071_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 248071_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:13:15.98 +40:10:24.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248100_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 248100_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 248128_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 248128_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 248142_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 248142_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:19:22.76 +40:08:55.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248155_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 248155_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:05:22.55 +42:17:42.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248179_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 248179_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:10:40.21 +40:02:55.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248393_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 248393_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
Rejecting candidate due to large distance (17.7") between the two second-epoch detections
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Considering the candidate 248423_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 248423_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:30:43.00 +39:52:01.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 217123_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 217123_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 110147_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
Preparing report for the candidate 110147_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
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Considering the candidate 102240_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
Preparing report for the candidate 102240_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
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Considering the candidate 69851_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
Preparing report for the candidate 69851_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
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Considering the candidate 224678_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 224678_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 24314_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
Preparing report for the candidate 24314_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
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Considering the candidate 46899_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 46899_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:18:18.99 +35:15:00.0 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 77826_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
Preparing report for the candidate 77826_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
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Considering the candidate 43591_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
Preparing report for the candidate 43591_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
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Considering the candidate 150482_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 150482_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 123486_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 123486_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:36:37.53 +39:42:30.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 225269_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 225269_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
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Considering the candidate 76522_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
Preparing report for the candidate 76522_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
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Considering the candidate 133126_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
Preparing report for the candidate 133126_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
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Considering the candidate 197558_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 197558_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:57:29.28 +41:11:02.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 17453_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 17453_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 04:56:18.75 +33:03:53.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53361_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
Preparing report for the candidate 53361_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
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Considering the candidate 78906_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 78906_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
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Considering the candidate 42169_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
Preparing report for the candidate 42169_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
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Considering the candidate 32333_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 32333_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 04:59:52.34 +33:59:08.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 95220_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 95220_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:07:56.98 +37:48:57.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72927_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 72927_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:26:54.62 +36:54:10.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193836_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
Preparing report for the candidate 193836_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
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Considering the candidate 49989_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
Preparing report for the candidate 49989_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
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Considering the candidate 30548_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 30548_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:28:49.03 +34:25:10.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33937_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
Preparing report for the candidate 33937_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
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Considering the candidate 77591_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 77591_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:08:33.65 +36:53:45.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 86818_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
Preparing report for the candidate 86818_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
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Considering the candidate 24263_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
Preparing report for the candidate 24263_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
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Considering the candidate 102689_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
Preparing report for the candidate 102689_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
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Considering the candidate 198845_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 198845_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:09:44.62 +40:44:25.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 222703_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 222703_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 213619_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 213619_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:38:03.76 +34:25:03.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 1.976 3449619536314095232 084.51613880730 +34.41736314146 11.1028 9.5975 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.976#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 41577_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 41577_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 192232_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 192232_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:32:37.61 +41:28:08.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 85254_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
Preparing report for the candidate 85254_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
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Considering the candidate 221531_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 221531_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:09:08.42 +37:40:43.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 0.358 188056242567734912 077.28499702999 +37.67876088689 11.8610 10.3830 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.358#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 49281_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 49281_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:38:22.06 +35:37:28.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 39924_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
Preparing report for the candidate 39924_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
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Considering the candidate 27418_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 27418_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:10:42.18 +33:57:16.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 44756_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
Preparing report for the candidate 44756_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
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Considering the candidate 221452_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 221452_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 133332_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 133332_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:10:20.35 +39:49:23.1 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 50292_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 50292_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:25:29.53 +35:35:43.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 79222_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
Preparing report for the candidate 79222_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
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Considering the candidate 114669_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 114669_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:20:15.03 +39:06:51.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 159098_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 159098_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
Rejecting candidate due to large distance (16.5") between the two second-epoch detections
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Considering the candidate 20904_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 20904_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 146725_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 146725_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 04:50:00.94 +39:55:56.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 73667_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
Preparing report for the candidate 73667_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
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Considering the candidate 176545_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 176545_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:27:47.17 +42:02:18.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 115354_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
Preparing report for the candidate 115354_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
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Considering the candidate 55043_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
Preparing report for the candidate 55043_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
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Considering the candidate 108410_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
Preparing report for the candidate 108410_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
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Considering the candidate 192838_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
Preparing report for the candidate 192838_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
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Considering the candidate 57731_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
Preparing report for the candidate 57731_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
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Considering the candidate 16031_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
Preparing report for the candidate 16031_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
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Considering the candidate 86440_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 86440_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:30:32.89 +37:44:47.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 49874_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
Preparing report for the candidate 49874_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
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Considering the candidate 42031_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
Preparing report for the candidate 42031_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
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Considering the candidate 219894_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 219894_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 85907_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 85907_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:30:38.63 +37:43:04.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 39993_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
Preparing report for the candidate 39993_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
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Considering the candidate 219654_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 219654_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
Rejecting candidate due to large distance (49.9") between the two second-epoch detections
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Considering the candidate 85851_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
Preparing report for the candidate 85851_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
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Considering the candidate 121239_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 121239_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 92668_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
Preparing report for the candidate 92668_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
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Considering the candidate 139440_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
Preparing report for the candidate 139440_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
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Considering the candidate 219153_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 219153_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
Rejecting candidate due to large distance (94.6") between the two second-epoch detections
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Considering the candidate 114580_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
Preparing report for the candidate 114580_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
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Considering the candidate 218915_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 218915_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 128590_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
Preparing report for the candidate 128590_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
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Considering the candidate 41258_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
Preparing report for the candidate 41258_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
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Considering the candidate 181995_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
Preparing report for the candidate 181995_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
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Considering the candidate 27184_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 27184_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:27:07.48 +34:08:59.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67315_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
Preparing report for the candidate 67315_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
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Considering the candidate 82064_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
Preparing report for the candidate 82064_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
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Considering the candidate 96748_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
Preparing report for the candidate 96748_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
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Considering the candidate 92016_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
Preparing report for the candidate 92016_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
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Considering the candidate 195170_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
Preparing report for the candidate 195170_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
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Considering the candidate 46614_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
Preparing report for the candidate 46614_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
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Considering the candidate 117999_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 117999_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:47:32.81 +39:27:53.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 111430_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 111430_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:41:55.85 +38:56:00.5 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 194777_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 194777_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:41:19.86 +41:19:11.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 44233_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 44233_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:20:55.61 +35:05:21.8 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 216627_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 216627_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 138230_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
Preparing report for the candidate 138230_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
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Considering the candidate 37082_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 37082_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 103006_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 103006_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:21:01.11 +38:28:04.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 26002_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 26002_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
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Considering the candidate 84748_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 84748_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:24:39.25 +37:23:04.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 40102_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 40102_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:25:12.91 +34:51:18.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 62623_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 62623_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:24:44.87 +36:11:59.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 50609_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 50609_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:26:54.30 +35:27:26.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 107835_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 107835_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:13:26.02 +38:28:58.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 138800_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 138800_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:19:09.86 +40:05:34.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 135410_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 135410_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:36:52.36 +40:10:53.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 35080_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 35080_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:27:38.89 +34:28:34.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 31857_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 31857_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:26:48.78 +34:23:31.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 39034_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 39034_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:13:20.74 +34:37:05.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 26464_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 26464_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:20:00.99 +33:57:30.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 33448_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 33448_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:16:18.21 +34:18:46.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 12616_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 12616_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:26:51.23 +33:15:44.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 22925_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 22925_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:19:00.14 +33:44:54.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 116001_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 116001_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:49:10.12 +39:10:48.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 17489_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 17489_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:18:10.77 +33:22:15.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 104499_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
Preparing report for the candidate 104499_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
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Considering the candidate 114368_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 114368_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 05:51:29.06 +39:08:52.1 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 19751_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431
The candidate 19751_fd_Aur-03-Q1b1x1_2026-07-12_05-15-00_20.00sec_-0.00C_LIGHTs_0431 did not pass the final checks
**** FOUND 04:57:00.23 +33:10:00.7 in the exclusion list exclusion_list_bbsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 5s
make_report_in_HTML.sh TOTAL: 57s
Prepared the HTML report for the field Aur-03-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
05:20:55.63 +35:05:21.4
05:18:19.01 +35:14:59.8
05:21:01.14 +38:28:04.6
05:41:55.89 +38:56:00.6
05:47:32.85 +39:27:53.1
05:10:20.38 +39:49:22.9
05:57:29.31 +41:11:02.9
05:45:01.83 +38:39:41.0
05:32:02.40 +38:38:23.6
05:20:36.57 +38:35:56.2
05:40:58.91 +38:58:51.0
05:30:18.67 +38:59:30.7
05:37:14.73 +39:16:27.9
05:30:24.07 +39:15:41.2
05:06:24.40 +39:32:46.2
05:24:55.85 +40:04:01.8
05:34:46.85 +40:24:26.7
05:57:27.49 +40:27:58.0
05:23:15.74 +33:32:07.8
05:54:43.03 +41:52:12.7
05:46:54.87 +41:24:30.6
05:32:06.00 +41:17:38.6
05:47:58.87 +41:17:44.9
05:13:11.52 +33:50:57.0
05:28:37.29 +34:02:29.4
05:28:50.48 +33:29:34.1
05:16:15.54 +34:27:17.1
05:17:30.61 +34:49:22.4
05:36:12.72 +35:03:05.6
05:18:56.99 +34:57:09.1
05:02:26.25 +34:39:46.2
05:00:49.35 +34:37:49.6
05:37:30.83 +35:17:00.7
05:26:35.54 +35:15:11.6
05:16:59.17 +35:14:10.8
05:26:53.89 +35:34:49.3
04:59:47.65 +35:03:04.6
05:06:30.50 +35:23:18.1
05:20:58.41 +35:48:43.1
05:16:02.97 +35:53:46.6
05:27:17.87 +36:39:05.8
05:24:50.75 +36:46:09.0
05:03:20.33 +36:34:50.8
05:17:46.91 +36:59:31.6
05:10:09.13 +36:56:11.9
05:31:11.28 +37:20:50.9
05:22:09.37 +37:23:14.8
05:40:07.75 +37:38:11.5
05:33:34.46 +37:43:25.2
05:08:17.26 +37:24:54.1
05:06:25.57 +37:34:30.5
05:20:07.41 +37:57:30.2
05:20:45.06 +38:10:49.4
########### Completed Aur-03-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 ####
05:47:32.85 +39:27:53.1
05:20:55.63 +35:05:21.4
05:41:55.89 +38:56:00.6
05:18:19.01 +35:14:59.8
05:10:20.38 +39:49:22.9
05:57:29.31 +41:11:02.9
05:21:01.14 +38:28:04.6
05:28:50.48 +33:29:34.1
05:30:18.67 +38:59:30.7
05:45:01.83 +38:39:41.0
05:24:50.75 +36:46:09.0
05:28:37.29 +34:02:29.4
05:10:09.13 +36:56:11.9
05:37:30.83 +35:17:00.7
05:17:46.91 +36:59:31.6
05:24:55.85 +40:04:01.8
05:06:30.50 +35:23:18.1
05:00:49.35 +34:37:49.6
05:32:06.00 +41:17:38.6
04:59:47.65 +35:03:04.6
05:16:15.54 +34:27:17.1
05:08:17.26 +37:24:54.1
05:13:11.52 +33:50:57.0
05:32:02.40 +38:38:23.6
05:40:07.75 +37:38:11.5
05:17:30.61 +34:49:22.4
05:26:35.54 +35:15:11.6
05:31:11.28 +37:20:50.9
05:03:20.33 +36:34:50.8
05:30:24.07 +39:15:41.2
05:20:58.41 +35:48:43.1
05:40:58.91 +38:58:51.0
05:46:54.87 +41:24:30.6
05:16:02.97 +35:53:46.6
05:23:15.74 +33:32:07.8
05:26:53.89 +35:34:49.3
05:02:26.25 +34:39:46.2
05:36:12.72 +35:03:05.6
05:33:34.46 +37:43:25.2
05:20:07.41 +37:57:30.2
05:57:27.49 +40:27:58.0
05:37:14.73 +39:16:27.9
05:06:24.40 +39:32:46.2
05:18:56.99 +34:57:09.1
05:54:43.03 +41:52:12.7
05:27:17.87 +36:39:05.8
05:22:09.37 +37:23:14.8
05:20:45.06 +38:10:49.4
05:06:25.57 +37:34:30.5
05:47:58.87 +41:17:44.9
05:16:59.17 +35:14:10.8
05:34:46.85 +40:24:26.7
05:20:36.57 +38:35:56.2
###################################################################################
05:47:32.85 +39:27:53.1 -- not an asteroid (will add it to exclusion list)
05:20:55.63 +35:05:21.4 -- not an asteroid (will add it to exclusion list)
05:41:55.89 +38:56:00.6 -- not an asteroid (will add it to exclusion list)
05:18:19.01 +35:14:59.8 -- not an asteroid (will add it to exclusion list)
05:10:20.38 +39:49:22.9 -- not an asteroid (will add it to exclusion list)
05:57:29.31 +41:11:02.9 -- not an asteroid (will add it to exclusion list)
05:21:01.14 +38:28:04.6 -- not an asteroid (will add it to exclusion list)
05:28:50.48 +33:29:34.1 -- asteroid (will NOT add it to exclusion list)
05:30:18.67 +38:59:30.7 -- not an asteroid (will add it to exclusion list)
05:45:01.83 +38:39:41.0 -- not an asteroid (will add it to exclusion list)
05:24:50.75 +36:46:09.0 -- not an asteroid (will add it to exclusion list)
05:28:37.29 +34:02:29.4 -- not an asteroid (will add it to exclusion list)
05:10:09.13 +36:56:11.9 -- not an asteroid (will add it to exclusion list)
05:37:30.83 +35:17:00.7 -- not an asteroid (will add it to exclusion list)
05:17:46.91 +36:59:31.6 -- not an asteroid (will add it to exclusion list)
05:24:55.85 +40:04:01.8 -- not an asteroid (will add it to exclusion list)
05:06:30.50 +35:23:18.1 -- not an asteroid (will add it to exclusion list)
05:00:49.35 +34:37:49.6 -- not an asteroid (will add it to exclusion list)
05:32:06.00 +41:17:38.6 -- not an asteroid (will add it to exclusion list)
04:59:47.65 +35:03:04.6 -- not an asteroid (will add it to exclusion list)
05:16:15.54 +34:27:17.1 -- not an asteroid (will add it to exclusion list)
05:08:17.26 +37:24:54.1 -- not an asteroid (will add it to exclusion list)
05:13:11.52 +33:50:57.0 -- not an asteroid (will add it to exclusion list)
05:32:02.40 +38:38:23.6 -- not an asteroid (will add it to exclusion list)
05:40:07.75 +37:38:11.5 -- not an asteroid (will add it to exclusion list)
05:17:30.61 +34:49:22.4 -- not an asteroid (will add it to exclusion list)
05:26:35.54 +35:15:11.6 -- not an asteroid (will add it to exclusion list)
05:31:11.28 +37:20:50.9 -- not an asteroid (will add it to exclusion list)
05:03:20.33 +36:34:50.8 -- not an asteroid (will add it to exclusion list)
05:30:24.07 +39:15:41.2 -- not an asteroid (will add it to exclusion list)
05:20:58.41 +35:48:43.1 -- not an asteroid (will add it to exclusion list)
05:40:58.91 +38:58:51.0 -- not an asteroid (will add it to exclusion list)
05:46:54.87 +41:24:30.6 -- not an asteroid (will add it to exclusion list)
05:16:02.97 +35:53:46.6 -- not an asteroid (will add it to exclusion list)
05:23:15.74 +33:32:07.8 -- not an asteroid (will add it to exclusion list)
05:26:53.89 +35:34:49.3 -- not an asteroid (will add it to exclusion list)
05:02:26.25 +34:39:46.2 -- not an asteroid (will add it to exclusion list)
05:36:12.72 +35:03:05.6 -- not an asteroid (will add it to exclusion list)
05:33:34.46 +37:43:25.2 -- not an asteroid (will add it to exclusion list)
05:20:07.41 +37:57:30.2 -- not an asteroid (will add it to exclusion list)
05:57:27.49 +40:27:58.0 -- not an asteroid (will add it to exclusion list)
05:37:14.73 +39:16:27.9 -- not an asteroid (will add it to exclusion list)
05:06:24.40 +39:32:46.2 -- not an asteroid (will add it to exclusion list)
05:18:56.99 +34:57:09.1 -- not an asteroid (will add it to exclusion list)
05:54:43.03 +41:52:12.7 -- not an asteroid (will add it to exclusion list)
05:27:17.87 +36:39:05.8 -- not an asteroid (will add it to exclusion list)
05:22:09.37 +37:23:14.8 -- not an asteroid (will add it to exclusion list)
05:20:45.06 +38:10:49.4 -- not an asteroid (will add it to exclusion list)
05:06:25.57 +37:34:30.5 -- not an asteroid (will add it to exclusion list)
05:47:58.87 +41:17:44.9 -- not an asteroid (will add it to exclusion list)
05:16:59.17 +35:14:10.8 -- not an asteroid (will add it to exclusion list)
05:34:46.85 +40:24:26.7 -- not an asteroid (will add it to exclusion list)
05:20:36.57 +38:35:56.2 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
04:59:47.65 +35:03:04.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:00:49.35 +34:37:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:02:26.25 +34:39:46.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:03:20.33 +36:34:50.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:06:24.40 +39:32:46.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:06:25.57 +37:34:30.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:06:30.50 +35:23:18.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:08:17.26 +37:24:54.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:10:09.13 +36:56:11.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:10:20.38 +39:49:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:13:11.52 +33:50:57.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:16:02.97 +35:53:46.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:16:15.54 +34:27:17.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:16:59.17 +35:14:10.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:30.61 +34:49:22.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:46.91 +36:59:31.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:19.01 +35:14:59.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:56.99 +34:57:09.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:20:07.41 +37:57:30.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:20:36.57 +38:35:56.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:20:45.06 +38:10:49.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:20:55.63 +35:05:21.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:20:58.41 +35:48:43.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:21:01.14 +38:28:04.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:22:09.37 +37:23:14.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:23:15.74 +33:32:07.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:24:50.75 +36:46:09.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:24:55.85 +40:04:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:26:35.54 +35:15:11.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:26:53.89 +35:34:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:27:17.87 +36:39:05.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:28:37.29 +34:02:29.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:30:18.67 +38:59:30.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:30:24.07 +39:15:41.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:31:11.28 +37:20:50.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:32:02.40 +38:38:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:32:06.00 +41:17:38.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:33:34.46 +37:43:25.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:34:46.85 +40:24:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:36:12.72 +35:03:05.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:14.73 +39:16:27.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:30.83 +35:17:00.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:40:07.75 +37:38:11.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:40:58.91 +38:58:51.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:41:55.89 +38:56:00.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:45:01.83 +38:39:41.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:46:54.87 +41:24:30.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:47:32.85 +39:27:53.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:47:58.87 +41:17:44.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:54:43.03 +41:52:12.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:27.49 +40:27:58.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:29.31 +41:11:02.9 -- 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)
04:59:47.65 +35:03:04.6 -- a known variable star
05:00:49.35 +34:37:49.6 -- a known variable star
05:02:26.25 +34:39:46.2 -- a known variable star
05:03:20.33 +36:34:50.8 -- a known variable star
05:06:24.40 +39:32:46.2 -- a known variable star
05:06:25.57 +37:34:30.5 -- a known variable star
05:06:30.50 +35:23:18.1 -- a known variable star
05:08:17.26 +37:24:54.1 -- a known variable star
05:10:09.13 +36:56:11.9 -- a known variable star
05:10:20.38 +39:49:22.9 -- a known variable star
05:13:11.52 +33:50:57.0 -- a known variable star
05:16:02.97 +35:53:46.6 -- a known variable star
05:16:15.54 +34:27:17.1 -- a known variable star
05:16:59.17 +35:14:10.8 -- a known variable star
05:17:30.61 +34:49:22.4 -- a known variable star
05:17:46.91 +36:59:31.6 -- a known variable star
05:18:19.01 +35:14:59.8 -- a known variable star
05:18:56.99 +34:57:09.1 -- a known variable star
05:20:07.41 +37:57:30.2 -- a known variable star
05:20:36.57 +38:35:56.2 -- a known variable star
05:20:45.06 +38:10:49.4 -- a known variable star
05:20:55.63 +35:05:21.4 -- a known variable star
05:20:58.41 +35:48:43.1 -- a known variable star
05:21:01.14 +38:28:04.6 -- a known variable star
05:22:09.37 +37:23:14.8 -- a known variable star
05:23:15.74 +33:32:07.8 -- a known variable star
05:24:50.75 +36:46:09.0 -- a known variable star
05:24:55.85 +40:04:01.8 -- a known variable star
05:26:35.54 +35:15:11.6 -- a known variable star
05:26:53.89 +35:34:49.3 -- a known variable star
05:27:17.87 +36:39:05.8 -- not a known variable star
05:28:37.29 +34:02:29.4 -- a known variable star
05:30:18.67 +38:59:30.7 -- a known variable star
05:30:24.07 +39:15:41.2 -- a known variable star
05:31:11.28 +37:20:50.9 -- a known variable star
05:32:02.40 +38:38:23.6 -- a known variable star
05:32:06.00 +41:17:38.6 -- a known variable star
05:33:34.46 +37:43:25.2 -- a known variable star
05:34:46.85 +40:24:26.7 -- a known variable star
05:36:12.72 +35:03:05.6 -- a known variable star
05:37:14.73 +39:16:27.9 -- a known variable star
05:37:30.83 +35:17:00.7 -- a known variable star
05:40:07.75 +37:38:11.5 -- a known variable star
05:40:58.91 +38:58:51.0 -- a known variable star
05:41:55.89 +38:56:00.6 -- a known variable star
05:45:01.83 +38:39:41.0 -- a known variable star
05:46:54.87 +41:24:30.6 -- a known variable star
05:47:32.85 +39:27:53.1 -- a known variable star
05:47:58.87 +41:17:44.9 -- a known variable star
05:54:43.03 +41:52:12.7 -- a known variable star
05:57:27.49 +40:27:58.0 -- a known variable star
05:57:29.31 +41:11:02.9 -- a known variable star
Found 1 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
52 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 ####
04:59:47.65 +35:03:04.6
05:00:49.35 +34:37:49.6
05:02:26.25 +34:39:46.2
05:03:20.33 +36:34:50.8
05:06:24.40 +39:32:46.2
05:06:25.57 +37:34:30.5
05:06:30.50 +35:23:18.1
05:08:17.26 +37:24:54.1
05:10:09.13 +36:56:11.9
05:10:20.38 +39:49:22.9
05:13:11.52 +33:50:57.0
05:16:02.97 +35:53:46.6
05:16:15.54 +34:27:17.1
05:16:59.17 +35:14:10.8
05:17:30.61 +34:49:22.4
05:17:46.91 +36:59:31.6
05:18:19.01 +35:14:59.8
05:18:56.99 +34:57:09.1
05:20:07.41 +37:57:30.2
05:20:36.57 +38:35:56.2
05:20:45.06 +38:10:49.4
05:20:55.63 +35:05:21.4
05:20:58.41 +35:48:43.1
05:21:01.14 +38:28:04.6
05:22:09.37 +37:23:14.8
05:23:15.74 +33:32:07.8
05:24:50.75 +36:46:09.0
05:24:55.85 +40:04:01.8
05:26:35.54 +35:15:11.6
05:26:53.89 +35:34:49.3
05:27:17.87 +36:39:05.8
05:28:37.29 +34:02:29.4
05:30:18.67 +38:59:30.7
05:30:24.07 +39:15:41.2
05:31:11.28 +37:20:50.9
05:32:02.40 +38:38:23.6
05:32:06.00 +41:17:38.6
05:33:34.46 +37:43:25.2
05:34:46.85 +40:24:26.7
05:36:12.72 +35:03:05.6
05:37:14.73 +39:16:27.9
05:37:30.83 +35:17:00.7
05:40:07.75 +37:38:11.5
05:40:58.91 +38:58:51.0
05:41:55.89 +38:56:00.6
05:45:01.83 +38:39:41.0
05:46:54.87 +41:24:30.6
05:47:32.85 +39:27:53.1
05:47:58.87 +41:17:44.9
05:54:43.03 +41:52:12.7
05:57:27.49 +40:27:58.0
05:57:29.31 +41:11:02.9
05:38:03.76 +34:25:03.9
05:09:08.42 +37:40:43.8
05:30:33.80 +33:00:24.3
####################################################
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461233.92668983 -observatory V36
07:26:40.21 +17:05:58.0 Mercury (5.6mag)
10:20:18.39 +11:45:54.7 Venus (-4.1mag)
04:30:19.69 +21:40:23.9 Mars (1.3mag)
08:18:33.83 +20:05:30.1 Jupiter (-1.8mag)
00:56:03.83 +03:21:12.3 Saturn (0.7mag)
04:07:37.65 +20:46:07.1 Uranus (5.8mag)
00:17:00.68 +00:20:28.8 Neptune (7.7mag)
20:30:43.43 -23:18:55.6 Pluto (14.4mag)
05:26:28.49 +27:24:03.3 Moon (-8.8mag)
-rw-r--r-- 1 apache apache 361 Jul 12 06:58 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461233.92668983:
08:18:40.81 +20:05:04.1 Io (6.1mag)
08:18:28.68 +20:05:49.5 Europa (6.3mag)
08:18:35.31 +20:05:21.3 Ganymede (5.6mag)
08:18:46.79 +20:04:38.5 Callisto (6.8mag)
08:16:59.62 +19:50:32.4 Himalia (15.7mag)
08:18:34.55 +20:05:28.2 Thebe (16.6mag)
08:16:20.51 +19:54:33.0 Elara (17.6mag)
08:22:09.89 +19:58:33.6 Pasiphae (17.8mag)
08:23:24.56 +20:10:53.1 Carme (19.0mag)
00:56:01.75 +03:20:44.4 Titan (8.5mag)
00:56:08.75 +03:21:03.6 Rhea (9.8mag)
00:55:30.89 +03:19:57.7 Iapetus (11.2mag)
00:56:04.22 +03:21:41.7 Hyperion (14.5mag)
00:56:01.77 +03:18:07.9 Phoebe (16.6mag)
-rw-r--r-- 1 apache apache 568 Jul 12 06:58 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461233.92668983:
17:48:38.12 -32:29:41.9 JWST
12:35:55.22 +51:31:34.6 Chandra
05:45:33.05 +36:33:48.8 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jul 12 06:58 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461233.92668983 -observatory V36
02:39:12.87 +14:40:29.0 17.9mag P/1996 R2 (Lagerkvist)
18:16:21.07 -34:25:08.9 13.7mag P/2010 H2 (Vales)
06:27:45.17 -68:10:23.1 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:01:31.62 +32:28:56.6 17.6mag C/2017 K2 (PANSTARRS)
01:59:23.30 +12:11:49.4 15.5mag P/2021 N1 (ZTF)
22:58:16.72 +32:16:50.7 17.3mag C/2022 E2 (ATLAS)
06:14:46.03 +26:54:28.2 16.7mag C/2022 N2 (PANSTARRS)
09:57:19.47 +29:41:17.0 16.8mag C/2022 QE78 (ATLAS)
09:11:04.54 +05:02:19.1 17.8mag C/2022 R6 (PANSTARRS)
18:05:57.45 +21:12:48.1 18.0mag C/2023 A3 (Tsuchinshan-ATLAS)
15:11:23.26 -11:26:08.1 17.7mag P/2023 B1 (PANSTARRS)
21:46:43.34 +67:36:19.1 17.8mag C/2023 H5 (Lemmon)
16:26:49.55 -10:17:42.4 13.9mag C/2023 R1 (PANSTARRS)
08:04:15.29 +65:49:13.1 17.9mag C/2024 A1 (ATLAS)
07:35:31.94 +30:06:33.0 14.7mag C/2024 E1 (Wierzchos)
15:15:20.04 +15:22:55.4 17.6mag C/2024 G6 (ATLAS)
19:38:39.72 +39:47:40.9 13.8mag C/2024 J3 (ATLAS)
21:45:25.37 +46:18:50.0 17.8mag C/2024 R4 (PANSTARRS)
04:51:35.84 -13:42:09.6 15.7mag C/2024 T5 (ATLAS)
06:36:17.49 +28:43:26.1 18.0mag C/2025 J1 (Borisov)
07:15:47.55 -13:04:27.8 16.6mag C/2025 R3 (PANSTARRS)
09:58:30.25 +22:20:51.3 17.6mag C/2025 V2 (Rankin)
12:45:19.06 +03:50:55.3 17.1mag C/2025 Y1 (ATLAS)
16:46:07.52 +79:09:23.2 17.3mag C/2026 A2 (Bok)
02:48:28.06 +45:19:47.4 16.7mag C/2026 B2 (Sun-Gao)
11:26:50.30 +04:54:39.5 17.0mag A/2026 E1
21:22:17.04 -15:49:25.1 7.2mag 10P/Tempel
11:14:25.88 -01:58:34.3 16.2mag 29P/Schwassmann-Wachmann
04:03:09.81 +29:46:43.9 17.9mag 47P/Ashbrook-Jackson
10:12:24.81 +13:21:00.2 17.0mag 63P/Wild
00:49:15.17 -05:04:12.7 15.5mag 65P/Gunn
08:33:25.50 +34:06:54.3 18.0mag 76P/West-Kohoutek-Ikemura
04:32:25.17 +20:17:06.7 13.7mag 78P/Gehrels
02:25:41.15 +10:53:43.3 16.2mag 88P/Howell
06:41:42.51 +30:24:38.3 15.7mag 93P/Lovas
04:27:44.43 +31:12:24.5 16.8mag 114P/Wiseman-Skiff
08:13:46.17 +30:28:17.6 15.2mag 123P/West-Hartley
10:52:00.34 +00:20:33.5 16.8mag 124P/Mrkos
04:55:03.83 +20:52:19.3 16.2mag 128P/Shoemaker-Holt
05:40:10.29 +19:41:49.8 17.8mag 131P/Mueller
00:02:05.93 +03:00:55.8 17.9mag 139P/Vaisala-Oterma
07:21:11.66 +16:34:16.2 15.8mag 141P-D/Machholz
03:17:43.08 -20:56:01.5 15.4mag 161P/Hartley-IRAS
05:40:32.49 +34:23:31.4 15.4mag 162P/SidingSpring
18:59:00.81 +16:22:26.1 14.6mag 169P/NEAT
01:45:58.91 +07:49:50.6 17.7mag 220P/McNaught
16:35:42.34 -08:28:05.4 17.1mag 235P/LINEAR
08:49:39.69 +33:06:27.7 17.9mag 240P/NEAT
20:41:15.68 -50:01:18.5 17.8mag 259P/Garradd
02:05:07.04 +13:03:58.0 15.7mag 260P/McNaught
05:43:31.48 +37:00:26.9 17.4mag 295P/LINEAR
15:06:30.91 +05:52:18.3 17.6mag 391P/Kowalski
08:36:28.11 +19:35:32.9 17.9mag 450P/LONEOS
07:55:01.62 +39:02:38.1 17.9mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.7K Jul 12 06:58 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
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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 06:58 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
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
20:05:42.563 -29:15:23.57 AT 2026tey 2026-07-06.28 22.7284
19:57:23.739 -26:50:39.25 AT 2026tex 2026-07-06.28 22.0768
20:17:33.319 -18:57:13.64 AT 2026tew 2026-07-06.29 22.7075
19:23:45.194 -19:41:24.47 AT 2026tev 2026-07-06.27 22.3458
20:07:43.974 -21:35:59.17 AT 2026teu 2026-07-06.28 22.8788
19:57:05.293 -24:56:17.03 AT 2026tet 2026-07-06.28 22.6654
19:56:26.112 -27:32:12.71 AT 2026tes 2026-07-06.28 22.4074
20:07:08.470 -28:14:32.90 AT 2026ter 2026-07-06.28 22.3947
00:36:20.815 -44:09:38.45 AT 2026teq 2026-07-06.42 22.7941
19:49:39.327 -27:34:48.80 AT 2026tep 2026-07-06.28 22.0721
19:41:45.859 -13:51:17.06 AT 2026teo 2026-07-06.29 21.9021
19:50:54.969 -16:24:44.71 AT 2026ten 2026-07-06.28 21.7555
19:20:22.817 -19:03:16.82 AT 2026tem 2026-07-06.27 22.8769
19:50:32.092 -27:38:04.96 AT 2026tel 2026-07-06.28 22.4265
-rw-r--r-- 1 apache apache 30K Jul 12 06:58 tns_transients_list.txt
