This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Aur-06-Q1b1x1_054643_TTUQ1b1x1_1787842_N2K9rk89
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 22.4486 2461243.9486 10.63 05:39:04.35 +29:55:34.3
178.40729 -0.68979 galactic Aur Second-epoch detections are separated by 0.6" and 5.4 pix
The object was found in VSX 1" LZ Aur
Type: LB
# Max. Min./Amp. JD0 Period
14.100 pg 15.400 pg M4:
The object was not found in astcheck.
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 05:39:04.35 +29:55:34.3: 11.58 +/- 0.01 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 05:39:04.35 +29:55:34.3: 11.54 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.56 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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
LZ Aur,2461243.9486,10.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
LZ Aur 20260722.4486 10.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 22.4486 2461243.9486 9.57 05:51:41.96 +28:18:24.7
181.22713 0.81860 galactic Tau Second-epoch detections are separated by 0.3" and 5.4 pix
The object was found in VSX 1" AZ Tau
Type: LB
# Max. Min./Amp. JD0 Period
11.540 V Y 0.380 V 2453298.90000 200.354756000000 M7-M8
The object was not found in astcheck.
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 05:51:41.96 +28:18:24.7: 10.49 +/- 0.00 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 05:51:41.96 +28:18:24.7: 10.50 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.49 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 22.4486* 05 51 41.96 +28 18 24.7 9.6 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
AZ Tau,2461243.9486,9.57,0.05,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
AZ Tau 20260722.4486 9.57CV 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 22.4486 2461243.9486 11.81 05:50:51.54 +33:33:39.2
176.61263 3.34353 galactic Aur Second-epoch detections are separated by 0.5" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.89 Julia -0 -1 1 11.5 0 0
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 05:50:51.54 +33:33:39.2: 16.13 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 05:50:51.54 +33:33:39.2: 16.11 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461243.9486,11.81,0.05,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 20260722.4486 11.81CV 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 22.4486 2461243.9486 11.21 05:59:47.26 +26:45:31.7
183.46788 1.58833 galactic Tau Second-epoch detections are separated by 1.0" and 5.4 pix
The object was found in VSX 1" BF Tau
Type: SRB
# Max. Min./Amp. JD0 Period
12.500 V 13.600 V 2452948.00000 194.900000000000 M5-M6
The object was not found in astcheck.
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 05:59:47.26 +26:45:31.7: 12.28 +/- 0.01 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 05:59:47.26 +26:45:31.7: 12.24 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.26 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 22.4486* 05 59 47.26 +26 45 31.7 11.2 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
BF Tau,2461243.9486,11.21,0.05,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
BF Tau 20260722.4486 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 22.4486 2461243.9486 11.85 06:17:05.51 +28:56:03.3
183.40372 5.98777 galactic Aur Second-epoch detections are separated by 1.4" and 5.1 pix
The object was found in VSX 1" NSVS J0617056+285602
Type: SR
# Max. Min./Amp. JD0 Period
14.528 g Y 0.817 g 2458567.92380 293.063510700000 M6
The object was not found in astcheck.
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 06:17:05.51 +28:56:03.3: 12.73 +/- 0.02 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 06:17:05.51 +28:56:03.3: 12.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 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 J0617056+285602,2461243.9486,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0617056+285602 20260722.4486 11.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 22.4486 2461243.9486 9.16 06:09:20.04 +26:31:43.3
184.71310 3.33635 galactic Gem Second-epoch detections are separated by 0.0" and 5.3 pix
The object was found in VSX 1" NSV 2843
Type: L
# Max. Min./Amp. JD0 Period
10.300 V 11.300 V 2452804.80000 99.500000000000 M6
The object was not found in astcheck.
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 06:09:20.04 +26:31:43.3: 10.13 +/- 0.00 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 06:09:20.04 +26:31:43.3: 10.12 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.13 +/- 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
NSV 2843,2461243.9486,9.16,0.05,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
NSV 2843 20260722.4486 9.16CV 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 22.4486 2461243.9486 10.82 06:03:26.73 +31:46:01.4
179.49424 4.74755 galactic Aur Second-epoch detections are separated by 1.5" and 5.2 pix
The object was found in VSX 2" ASASSN-V J060326.69+314603.3
Type: SR
# Max. Min./Amp. JD0 Period
11.600 V 12.070 V 2457290.10000 481.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 06:03:26.73 +31:46:01.4: 11.79 +/- 0.01 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 06:03:26.73 +31:46:01.4: 11.77 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.78 +/- 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 J060326.69+314603.3,2461243.9486,10.82,0.05,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 J060326.69+314603.3 20260722.4486 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 22.4486 2461243.9486 12.23 06:08:09.46 +31:08:02.6
180.53775 5.32211 galactic Aur Second-epoch detections are separated by 1.2" and 5.3 pix
The object was found in VSX 9" NSVS J0608096+310754
Type: L:
# Max. Min./Amp. JD0 Period
11.141 R1 Y 0.379 R1 121.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 06:08:09.46 +31:08:02.6: 13.18 +/- 0.02 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 06:08:09.46 +31:08:02.6: 13.22 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0608096+310754,2461243.9486,12.23,0.05,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 J0608096+310754 20260722.4486 12.23CV 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 22.4486 2461243.9486 11.93 06:25:39.14 +31:50:16.1
181.64628 8.95453 galactic Aur Second-epoch detections are separated by 1.4" and 5.4 pix
The object was found in VSX 1" GSC 02421-00613
Type: IB
# Max. Min./Amp. JD0 Period
10.900 R1 11.150 R1
The object was not found in astcheck.
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 06:25:39.14 +31:50:16.1: 12.97 +/- 0.02 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 06:25:39.14 +31:50:16.1: 12.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.97 +/- 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
GSC 02421-00613,2461243.9486,11.93,0.05,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 02421-00613 20260722.4486 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 22.4486 2461243.9486 11.70 06:01:22.02 +28:33:04.1
182.08281 2.77964 galactic Aur Second-epoch detections are separated by 0.6" and 5.2 pix
The object was found in VSX 1" BP Aur
Type: LB
# Max. Min./Amp. JD0 Period
13.900 pg 14.900 pg 306.000000000000 M6.5
The object was found in astcheck.1463 Nordenmarkia 430 -158 458 16.1 -0 0
NOTE: the measured brightness disagrees with the predicted asteroid brightness, but the matched variable star above likely accounts for this object.
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 06:01:22.02 +28:33:04.1: 12.62 +/- 0.02 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 06:01:22.02 +28:33:04.1: 12.61 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.61 +/- 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
BP Aur,2461243.9486,11.70,0.05,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
BP Aur 20260722.4486 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 22.4486 2461243.9486 10.39 06:08:45.08 +25:51:18.7
185.24092 2.89713 galactic Gem Second-epoch detections are separated by 0.3" and 5.4 pix
The object was found in VSX 1" V0379 Gem
Type: SRB
# Max. Min./Amp. JD0 Period
11.300 V 12.400 V 2452810.70000 149.000000000000 M5III
The object was found in astcheck.1081 Reseda -213 -261 337 16.8 0 0
NOTE: the measured brightness disagrees with the predicted asteroid brightness, but the matched variable star above likely accounts for this object.
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 06:08:45.08 +25:51:18.7: 11.37 +/- 0.01 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 06:08:45.08 +25:51:18.7: 11.37 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.37 +/- 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
V0379 Gem,2461243.9486,10.39,0.05,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
V0379 Gem 20260722.4486 10.39CV 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 22.4486 2461243.9486 11.23 06:08:59.52 +27:55:02.2
183.45667 3.93777 galactic Gem Second-epoch detections are separated by 1.0" and 5.2 pix
The object was found in VSX 1" ASASSN-V J060859.62+275502.7
Type: SR
# Max. Min./Amp. JD0 Period
12.230 V 12.680 V 2458586.84130 54.543637800000
The object was not found in astcheck.
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 06:08:59.52 +27:55:02.2: 12.17 +/- 0.01 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 06:08:59.52 +27:55:02.2: 12.16 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.17 +/- 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 J060859.62+275502.7,2461243.9486,11.23,0.05,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
ASASSN-V J060859.62+275502.7 20260722.4486 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 22.4486 2461243.9486 10.28 05:33:49.91 +26:38:06.4
180.56462 -3.43106 galactic Tau Second-epoch detections are separated by 0.1" and 5.5 pix
The object was found in VSX 3" NSVS 6927263
Type: SR
# Max. Min./Amp. JD0 Period
13.797 g Y 0.924 g 2458632.41590 479.074108400000 M6
The object was not found in astcheck.
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 05:33:49.91 +26:38:06.4: 11.27 +/- 0.01 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 05:33:49.91 +26:38:06.4: 11.27 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.27 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 22.4486* 05 33 49.91 +26 38 06.4 10.3 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 6927263,2461243.9486,10.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 6927263 20260722.4486 10.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 22.4486 2461243.9486 11.65 06:07:04.47 +25:40:36.7
185.21412 2.48046 galactic Gem Second-epoch detections are separated by 1.3" and 5.1 pix
The object was found in VSX 1" ASAS J060704+2540.6
Type: MISC
# Max. Min./Amp. JD0 Period
12.820 V Y 0.360 V 2452860.90000 76.656472000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 06:07:04.47 +25:40:36.7: 12.58 +/- 0.02 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 06:07:04.47 +25:40:36.7: 12.54 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.56 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J060704+2540.6,2461243.9486,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J060704+2540.6 20260722.4486 11.65CV 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 22.4486 2461243.9486 10.86 05:49:48.92 +25:25:25.0
183.48888 -1.01839 galactic Tau Second-epoch detections are separated by 0.7" and 5.5 pix
The object was found in VSX 2" AY Tau
Type: LB
# Max. Min./Amp. JD0 Period
11.540 V Y 0.660 V 2452849.50000 88.278568000000 M5
The object was not found in astcheck.
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 05:49:48.92 +25:25:25.0: 11.97 +/- 0.01 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 05:49:48.92 +25:25:25.0: 11.90 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.93 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 22.4486* 05 49 48.92 +25 25 25.0 10.9 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
AY Tau,2461243.9486,10.86,0.05,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
AY Tau 20260722.4486 10.86CV 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 22.4486 2461243.9486 12.09 05:49:34.61 +27:15:26.4
181.88811 -0.12215 galactic Tau Second-epoch detections are separated by 1.2" and 5.5 pix
The object was found in VSX 1" ASASSN-V J054934.66+271527.0
Type: SR
# Max. Min./Amp. JD0 Period
13.590 V 13.720 V 2457612.00000 261.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 05:49:34.61 +27:15:26.4: 13.16 +/- 0.03 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 05:49:34.61 +27:15:26.4: 13.11 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 22.4486* 05 49 34.61 +27 15 26.4 12.1 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J054934.66+271527.0,2461243.9486,12.09,0.05,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 J054934.66+271527.0 20260722.4486 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 22.4486 2461243.9486 12.40 05:44:22.61 +31:10:31.9
177.94955 0.93974 galactic Aur Second-epoch detections are separated by 3.3" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.250 Bettina -2 1 2 13.3 0 0
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 05:44:22.61 +31:10:31.9: 14.74 +/- 0.11 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 05:44:22.61 +31:10:31.9: 14.57 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.64 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin 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,2461243.9486,12.40,0.05,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
VARIABLE_NAME 20260722.4486 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 22.4486 2461243.9486 11.82 06:09:43.38 +25:12:22.8
185.91587 2.77621 galactic Gem Second-epoch detections are separated by 0.5" and 5.2 pix
The object was found in VSX 1" ASASSN-V J060943.37+251222.1
Type: L
# Max. Min./Amp. JD0 Period
13.130 V 13.570 V
The object was not found in astcheck.
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 06:09:43.38 +25:12:22.8: 12.84 +/- 0.02 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 06:09:43.38 +25:12:22.8: 12.84 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 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 J060943.37+251222.1,2461243.9486,11.82,0.05,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 J060943.37+251222.1 20260722.4486 11.82CV 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 22.4486 2461243.9486 12.73 05:50:37.25 +31:42:40.4
178.17978 2.35663 galactic Aur Second-epoch detections are separated by 2.2" and 4.8 pix
The object was found in VSX 1" IRAS 05473+3141
Type: SR
# Max. Min./Amp. JD0 Period
13.037 r Y 0.700 r 2458495.07020 156.568875400000 M6
The object was not found in astcheck.
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 05:50:37.25 +31:42:40.4: 13.97 +/- 0.05 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 05:50:37.25 +31:42:40.4: 13.96 +/- 0.05 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
IRAS 05473+3141,2461243.9486,12.73,0.05,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
IRAS 05473+3141 20260722.4486 12.73CV 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 22.4486 2461243.9486 11.38 05:59:02.03 +32:58:47.1
177.97565 4.53026 galactic Aur Second-epoch detections are separated by 0.6" and 5.2 pix
The object was found in VSX 1" NSVS 7007480
Type: SR
# Max. Min./Amp. JD0 Period
14.130 g Y 0.507 g 2458352.34600 119.588109400000
The object was not found in astcheck.
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 05:59:02.03 +32:58:47.1: 12.42 +/- 0.01 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 05:59:02.03 +32:58:47.1: 12.40 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.41 +/- 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 7007480,2461243.9486,11.38,0.05,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
NSVS 7007480 20260722.4486 11.38CV 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 22.4486 2461243.9486 12.32 06:01:25.27 +33:26:00.4
177.82528 5.18810 galactic Aur Second-epoch detections are separated by 1.2" and 5.4 pix
The object was found in VSX 3" NSVS J0601252+332603
Type: L:
# Max. Min./Amp. JD0 Period
11.307 R1 Y 0.465 R1 228.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 06:01:25.27 +33:26:00.4: 13.50 +/- 0.04 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 06:01:25.27 +33:26:00.4: 13.44 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.47 +/- 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 J0601252+332603,2461243.9486,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0601252+332603 20260722.4486 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 22.4486 2461243.9486 11.37 05:48:40.17 +26:28:28.7
182.45498 -0.69855 galactic Tau Second-epoch detections are separated by 1.8" and 5.7 pix
The object was found in VSX 2" V0422 Tau
Type: LB
# Max. Min./Amp. JD0 Period
15.500 pg 16.100 pg M7
ATTENTION: measured mag 11.37 is 4.1 mag brighter than the VSX record maximum brightness 15.50 - 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 found in astcheck.2725 David Bender 58 522 526 16.4 -0 0
ATTENTION: measured mag 11.37 is 5.0 mag brighter than the predicted asteroid brightness 16.4 - the transient may be an unrelated new object!
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 05:48:40.17 +26:28:28.7: 12.39 +/- 0.01 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 05:48:40.17 +26:28:28.7: 12.37 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.38 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 22.4486* 05 48 40.17 +26 28 28.7 11.4 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0422 Tau,2461243.9486,11.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0422 Tau 20260722.4486 11.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 22.4486 2461243.9486 11.26 06:30:54.31 +27:45:39.4
185.85078 8.15935 galactic Gem Second-epoch detections are separated by 0.9" and 5.1 pix
The object was found in VSX 2" ASAS J063054+2745.7
Type: MISC
# Max. Min./Amp. JD0 Period
12.540 V Y 0.820 V 2453024.70000 127.233353000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 06:30:54.31 +27:45:39.4: 12.30 +/- 0.01 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 06:30:54.31 +27:45:39.4: 12.32 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.31 +/- 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
ASAS J063054+2745.7,2461243.9486,11.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J063054+2745.7 20260722.4486 11.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 22.4486 2461243.9486 12.82 06:02:50.44 +34:41:47.7
176.86006 6.05945 galactic Aur Second-epoch detections are separated by 2.3" and 4.8 pix
The object was found in VSX 4" NSVS J0602506+344144
Type: L:
# Max. Min./Amp. JD0 Period
11.925 R1 Y 0.708 R1 85.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 06:02:50.44 +34:41:47.7: 14.13 +/- 0.06 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 06:02:50.44 +34:41:47.7: 13.95 +/- 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
NSVS J0602506+344144,2461243.9486,12.82,0.05,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
NSVS J0602506+344144 20260722.4486 12.82CV 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 22.4486 2461243.9486 11.96 05:57:39.56 +27:33:47.9
182.53412 1.57901 galactic Tau Second-epoch detections are separated by 1.7" and 5.3 pix
The object was found in VSX 1" ASASSN-V J055739.57+273349.2
Type: SR
# Max. Min./Amp. JD0 Period
14.579 g Y 0.447 g 2458428.05100 103.592762800000
The object was not found in astcheck.
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 05:57:39.56 +27:33:47.9: 13.02 +/- 0.02 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 05:57:39.56 +27:33:47.9: 13.04 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 22.4486* 05 57 39.56 +27 33 47.9 12.0 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J055739.57+273349.2,2461243.9486,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J055739.57+273349.2 20260722.4486 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 22.4486 2461243.9486 11.79 06:10:18.22 +32:03:09.6
179.94458 6.16136 galactic Aur Second-epoch detections are separated by 0.3" and 5.2 pix
The object was found in VSX 2" V0577 Aur
Type: SR:
# Max. Min./Amp. JD0 Period
12.700 V 13.500 V 419.000000000000 C
The object was not found in astcheck.
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 06:10:18.22 +32:03:09.6: 12.72 +/- 0.02 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 06:10:18.22 +32:03:09.6: 12.72 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.72 +/- 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
V0577 Aur,2461243.9486,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0577 Aur 20260722.4486 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 22.4486 2461243.9486 10.62 06:19:09.17 +32:18:41.0
180.59119 7.93925 galactic Aur Second-epoch detections are separated by 0.8" and 5.3 pix
The object was found in VSX 3" ASASSN-V J061909.17+321843.8
Type: L
# Max. Min./Amp. JD0 Period
11.580 V 12.300 V
The object was not found in astcheck.
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 06:19:09.17 +32:18:41.0: 11.58 +/- 0.01 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 06:19:09.17 +32:18:41.0: 11.59 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.59 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J061909.17+321843.8,2461243.9486,10.62,0.05,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 J061909.17+321843.8 20260722.4486 10.62CV 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 22.4486 2461243.9486 11.30 05:52:52.97 +29:50:15.6
180.04078 1.82040 galactic Aur Second-epoch detections are separated by 0.5" and 5.3 pix
The object was found in VSX 1" ASASSN-V J055253.00+295016.8
Type: L
# Max. Min./Amp. JD0 Period
12.550 V 12.960 V
The object was not found in astcheck.
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 05:52:52.97 +29:50:15.6: 12.23 +/- 0.01 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 05:52:52.97 +29:50:15.6: 12.21 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.22 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin 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 J055253.00+295016.8,2461243.9486,11.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J055253.00+295016.8 20260722.4486 11.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 22.4486 2461243.9486 12.22 06:15:37.37 +29:27:29.3
182.78743 5.94879 galactic Aur Second-epoch detections are separated by 2.7" and 4.8 pix
The object was found in VSX 2" ASASSN-V J061537.20+292729.9
Type: SR
# Max. Min./Amp. JD0 Period
13.800 V 14.430 V 2457644.10000 82.600000000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 06:15:37.37 +29:27:29.3: 13.48 +/- 0.04 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 06:15:37.37 +29:27:29.3: 13.44 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.46 +/- 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 J061537.20+292729.9,2461243.9486,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J061537.20+292729.9 20260722.4486 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 22.4486 2461243.9486 10.45 05:44:31.11 +30:40:39.2
178.38992 0.70519 galactic Aur Second-epoch detections are separated by 0.5" and 5.3 pix
The object was found in VSX 0" FQ Aur
Type: LB
# Max. Min./Amp. JD0 Period
13.500 pg 14.100 pg M3
The object was not found in astcheck.
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 05:44:31.11 +30:40:39.2: 11.45 +/- 0.01 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 05:44:31.11 +30:40:39.2: 11.43 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.44 +/- 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
FQ Aur,2461243.9486,10.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
FQ Aur 20260722.4486 10.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461093.61992316 22.02.2026 02:52:31.361 /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits
First image: 2461093.61992316 22.02.2026 02:52:31.361 /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits
Last image: 2461243.94885956 22.07.2026 10:46:11.466 /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Aur-06-Q1b1x1_054643_TTUQ1b1x1_1787842_N2K9rk89/fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 6
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.72
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: 13 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): 25208
Objects passed selection criteria: 25023
Measurements per detected object (mean, median, min, max): 2.4 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.4 2.0 2 4
Average stars detected per image: 15985
Average stars matched: 15479 (96.8345 %)
Memory usage VmPeak: 132560 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Jul 21 15:05:04 CDT 2026
VaST build number 1.0rc89-162-g0b3e9b13
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Jul 22 06:07:00 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: 2461093.61992316 22.02.2026 02:52:31.361 /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits
First image: 2461093.61992316 22.02.2026 02:52:31.361 /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits
Last image: 2461243.94885956 22.07.2026 10:46:11.466 /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Aur-06-Q1b1x1_054643_TTUQ1b1x1_1787842_N2K9rk89/fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 113
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.36
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 54 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): 192970
Objects passed selection criteria: 192295
Measurements per detected object (mean, median, min, max): 2.4 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.4 2.0 2 4
Average stars detected per image: 123352
Average stars matched: 118259 (95.8708 %)
Memory usage VmPeak: 1954344 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Jul 21 15:05:04 CDT 2026
VaST build number 1.0rc89-162-g0b3e9b13
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Jul 22 06:15:31 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 --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Aur-06-Q1b1x1_054643_TTUQ1b1x1_1787842_N2K9rk89/fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Aur-06-Q1b1x1_054643_TTUQ1b1x1_1787842_N2K9rk89/fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits
SExtractor catalog cache: saved Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits.cat to cache
SExtractor catalog cache: saved Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.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-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Aur-06-Q1b1x1_054643_TTUQ1b1x1_1787842_N2K9rk89/fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Aur-06-Q1b1x1_054643_TTUQ1b1x1_1787842_N2K9rk89/fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461243.94826677
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits exists and is non-empty
Saving wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits to local_wcs_cache/
'wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits' -> 'local_wcs_cache/wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits'
wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits exists and is non-empty
Saving wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits to local_wcs_cache/
'wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits' -> 'local_wcs_cache/wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits'
wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits exists and is non-empty
Saving wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits to local_wcs_cache/
'wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits' -> 'local_wcs_cache/wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits'
wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits exists and is non-empty
Saving wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits to local_wcs_cache/
'wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits' -> 'local_wcs_cache/wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits (1st reference image)
verification OK: wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits
Image size: 941.5'x626.9' 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: 06:00:00.480 +29:59:52.07 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-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits (1st new image)
verification OK: wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits
Image size: 944.6'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:59:51.679 +30:03:49.56 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 06:00:00.480 +29:59:52.07
Second-epoch image center 05:59:51.679 +30:03:49.56
Angular distance between the image centers 0.0732 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits (2nd new image)
verification OK: wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits
Image size: 944.5'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:59:54.014 +30:03:58.51 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 06:00:00.480 +29:59:52.07
Second-epoch image center 05:59:54.014 +30:03:58.51
Angular distance between the image centers 0.0723 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 05:59:51.679 +30:03:49.56
Second-epoch second image center 05:59:54.014 +30:03:58.51
Angular distance between the image centers 0.00878 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-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits &> /tmp/tmp.LHuoPX1qBR
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits &> /tmp/tmp.lF0unDvbeJ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Aur-06-Q1b1x1_054643_TTUQ1b1x1_1787842_N2K9rk89/fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits &> /tmp/tmp.ueTyrtyAAI
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Aur-06-Q1b1x1_054643_TTUQ1b1x1_1787842_N2K9rk89/fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Aur-06-Q1b1x1_054643_TTUQ1b1x1_1787842_N2K9rk89/fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits &> /tmp/tmp.XhTl65fSuE
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Aur-06-Q1b1x1_054643_TTUQ1b1x1_1787842_N2K9rk89/fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.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-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits and wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.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-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits and wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits.wcscat
Found non-empty wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits and wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits.wcscat
The reference image (wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits) and catalog (wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits.wcscat) found
'wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits.wcscat' -> 'wcsmag.cat'
Read 27193 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 80.5801 to 99.6659 deg, Dec +24.3425 to +35.3069 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 80.5801 to 99.6659 deg, Dec 24.3425 to 35.3069 deg
Loaded 17091 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): 11926 out of 13489 total matches.
Matched with Tycho-2 13489 out of 27193 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.946450
a=0.000000 b=1.000000 c=22.946450
From vast_summary.log: estimated ref. image limiting mag.: -7.72
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 27193 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 80.5801 to 99.6659 deg, Dec +24.3425 to +35.3069 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 80.5801 to 99.6659 deg, Dec 24.3425 to 35.3069 deg
Loaded 17091 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): 11926 out of 13489 total matches.
Matched with Tycho-2 13489 out of 27193 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits:
Forced-photometry filter: calibrated wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits -> calib.txt_param_ref_wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits (aperture=6.1)
Read 27141 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 80.5948 to 99.6661 deg, Dec +24.3432 to +35.3120 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 80.5948 to 99.6661 deg, Dec 24.3432 to 35.3120 deg
Loaded 17084 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): 12065 out of 13603 total matches.
Matched with Tycho-2 13603 out of 27141 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits:
Forced-photometry filter: calibrated wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits -> calib.txt_param_ref_wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits (aperture=6.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 6 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits
2.1 pix Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits
3.5 pix fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits
3.5 pix fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits
2.1 pix wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits
2.1 pix wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits
Limiting magnitude estimates:
15.2 mag. Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits
15.2 mag. Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits
13.0 mag. fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits
12.9 mag. fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits
All-image limiting magnitude estimate: 12.9 (SNR ) 10.5 (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.LHuoPX1qBR (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_2026-07-22_CI_Aur-06-Q1b1x1_054643_TTUQ1b1x1_1787842_N2K9rk89/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.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-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits' -> 'wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits
WCS_IMAGE_NAME=wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits
WCS-calibrated image found: wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits
Checking if the catalog wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits.wcscat corresponding to the image wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits alredy exist and is non-empty...
Catalog wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits.wcscat corresponding to the image wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits
WCS catalog name: wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.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=3136, bad_region=0, passed=27193
Got 27193 stars (including 24022 good ones) from the SExtractor catalog wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits.wcscat
util/solve_plate_with_UCAC5 got 27193 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 911 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 25972 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 25972 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 25972 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 934 stars left (next iteration limit 1027)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits N_match=934 sigma_overall_arcsec=0.513 sigma_q1_arcsec=0.542 sigma_q2_arcsec=0.478 sigma_q3_arcsec=0.516 sigma_q4_arcsec=0.455 n_q1=182 n_q2=276 n_q3=215 n_q4=261 worst_quadrant_to_overall_ratio=1.055
The image catalog is written to wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits -region wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.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.lF0unDvbeJ (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_2026-07-22_CI_Aur-06-Q1b1x1_054643_TTUQ1b1x1_1787842_N2K9rk89/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.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-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits' -> 'wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits
WCS_IMAGE_NAME=wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits
WCS-calibrated image found: wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits
Checking if the catalog wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits.wcscat corresponding to the image wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits alredy exist and is non-empty...
Catalog wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits.wcscat corresponding to the image wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits
WCS catalog name: wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.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=3121, bad_region=0, passed=27141
Got 27141 stars (including 23994 good ones) from the SExtractor catalog wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits.wcscat
util/solve_plate_with_UCAC5 got 27141 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 922 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 26212 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 26212 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 26213 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 937 stars left (next iteration limit 1030)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits N_match=937 sigma_overall_arcsec=0.486 sigma_q1_arcsec=0.552 sigma_q2_arcsec=0.429 sigma_q3_arcsec=0.463 sigma_q4_arcsec=0.422 n_q1=187 n_q2=281 n_q3=208 n_q4=261 worst_quadrant_to_overall_ratio=1.136
The image catalog is written to wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits -region wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.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.ueTyrtyAAI (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_2026-07-22_CI_Aur-06-Q1b1x1_054643_TTUQ1b1x1_1787842_N2K9rk89/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Aur-06-Q1b1x1_054643_TTUQ1b1x1_1787842_N2K9rk89/fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Aur-06-Q1b1x1_054643_TTUQ1b1x1_1787842_N2K9rk89/fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Aur-06-Q1b1x1_054643_TTUQ1b1x1_1787842_N2K9rk89/fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Aur-06-Q1b1x1_054643_TTUQ1b1x1_1787842_N2K9rk89/fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Aur-06-Q1b1x1_054643_TTUQ1b1x1_1787842_N2K9rk89/fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.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_2026-07-22_CI_Aur-06-Q1b1x1_054643_TTUQ1b1x1_1787842_N2K9rk89/fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits
WCS_IMAGE_NAME=wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits
WCS-calibrated image found: wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits
Checking if the catalog wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits.wcscat corresponding to the image wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits.wcscat corresponding to the image wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Aur-06-Q1b1x1_054643_TTUQ1b1x1_1787842_N2K9rk89/fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits
WCS catalog name: wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.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=271, bad_region=0, passed=5112
Got 5112 stars (including 4836 good ones) from the SExtractor catalog wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits.wcscat
util/solve_plate_with_UCAC5 got 5112 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 944.6'
Seting catalog search parameters based on the expected field of view 944.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013119 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010496 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 629 (Dec 24.3 to 35.5)
Done reading UCAC5 zone files...
Matched 929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 924 matched stars entering correct_measured_positions(), 889 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 924 matched stars entering correct_measured_positions(), 4910 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 629 (Dec 24.3 to 35.5)
Done reading UCAC5 zone files...
Matched 928 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 923 matched stars entering correct_measured_positions(), 4909 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Accuracy estimation diagnostic: 923 matched stars entering correct_measured_positions(), 4909 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Excluding outliers - 923 stars left (next iteration limit 1016)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits N_match=923 sigma_overall_arcsec=0.481 sigma_q1_arcsec=0.474 sigma_q2_arcsec=0.640 sigma_q3_arcsec=0.399 sigma_q4_arcsec=0.483 n_q1=250 n_q2=160 n_q3=332 n_q4=181 worst_quadrant_to_overall_ratio=1.329
The image catalog is written to wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Aur-06-Q1b1x1_054643_TTUQ1b1x1_1787842_N2K9rk89/fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits -region wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.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.XhTl65fSuE (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_2026-07-22_CI_Aur-06-Q1b1x1_054643_TTUQ1b1x1_1787842_N2K9rk89/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Aur-06-Q1b1x1_054643_TTUQ1b1x1_1787842_N2K9rk89/fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Aur-06-Q1b1x1_054643_TTUQ1b1x1_1787842_N2K9rk89/fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Aur-06-Q1b1x1_054643_TTUQ1b1x1_1787842_N2K9rk89/fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Aur-06-Q1b1x1_054643_TTUQ1b1x1_1787842_N2K9rk89/fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Aur-06-Q1b1x1_054643_TTUQ1b1x1_1787842_N2K9rk89/fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.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_2026-07-22_CI_Aur-06-Q1b1x1_054643_TTUQ1b1x1_1787842_N2K9rk89/fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits
WCS_IMAGE_NAME=wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits
WCS-calibrated image found: wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits
Checking if the catalog wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits.wcscat corresponding to the image wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits.wcscat corresponding to the image wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Aur-06-Q1b1x1_054643_TTUQ1b1x1_1787842_N2K9rk89/fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits
WCS catalog name: wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.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=264, bad_region=0, passed=4858
Got 4858 stars (including 4591 good ones) from the SExtractor catalog wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits.wcscat
util/solve_plate_with_UCAC5 got 4858 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 944.5'
Seting catalog search parameters based on the expected field of view 944.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013118 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010494 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 629 (Dec 24.3 to 35.5)
Done reading UCAC5 zone files...
Matched 929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 925 matched stars entering correct_measured_positions(), 890 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 925 matched stars entering correct_measured_positions(), 4651 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 629 (Dec 24.3 to 35.5)
Done reading UCAC5 zone files...
Matched 929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 924 matched stars entering correct_measured_positions(), 4656 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Accuracy estimation diagnostic: 924 matched stars entering correct_measured_positions(), 4656 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 924 stars left (next iteration limit 1017)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits N_match=924 sigma_overall_arcsec=0.502 sigma_q1_arcsec=0.469 sigma_q2_arcsec=0.631 sigma_q3_arcsec=0.421 sigma_q4_arcsec=0.574 n_q1=245 n_q2=166 n_q3=333 n_q4=180 worst_quadrant_to_overall_ratio=1.257
The image catalog is written to wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Aur-06-Q1b1x1_054643_TTUQ1b1x1_1787842_N2K9rk89/fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits -region wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.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-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits sigma_overall=0.513 worst_q_ratio=1.055
ref2=Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits sigma_overall=0.486 worst_q_ratio=1.136
new1=fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits sigma_overall=0.481 worst_q_ratio=1.329
new2=fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits sigma_overall=0.502 worst_q_ratio=1.257
reference average sigma_overall=0.4995 worst_q_ratio=1.0955
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056_astrometric_residuals.png (934 matched stars from wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.46 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057_astrometric_residuals.png (937 matched stars from wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.42 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424_astrometric_residuals.png (923 matched stars from wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.43 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425_astrometric_residuals.png (924 matched stars from wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.44 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Aur-06-Q1b1x1_054643_TTUQ1b1x1_1787842_N2K9rk89/wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits'
Saving fully-calibrated image wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Aur-06-Q1b1x1_054643_TTUQ1b1x1_1787842_N2K9rk89/wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits'
Preparing the HTML report for the field Aur-06-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 05:39:04.35 +29:55:34.3: 11.58 +/- 0.01 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 05:51:41.96 +28:18:24.7: 10.49 +/- 0.00 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 05:39:04.35 +29:55:34.3: 11.54 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.56 +/- 0.01
Forced photometry filter KEPT candidate at 05:39:04.35 +29:55:34.3: ref_mag=11.56 +/- 0.01 new_mean_mag=10.6308 delta=0.93 (need > 0.90)
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 05:51:41.96 +28:18:24.7: 10.50 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.49 +/- 0.00
Forced photometry filter KEPT candidate at 05:51:41.96 +28:18:24.7: ref_mag=10.49 +/- 0.00 new_mean_mag=9.5700 delta=0.92 (need > 0.90)
Adding exclusion_list_local.txt__out13666.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17578.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
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Considering the candidate 13666_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
Preparing report for the candidate 13666_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
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Considering the candidate 08609_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 08609_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 06:33:17.04 +31:35:29.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 17096_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 17096_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 06:04:17.03 +28:29:01.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 17578_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
Preparing report for the candidate 17578_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
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Considering the candidate 09704_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 09704_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 06:09:57.73 +31:24:25.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 13391_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 13391_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 05:37:46.34 +30:03:47.2 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 10s
Prepared the HTML report for the field Aur-06-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
05:39:04.35 +29:55:34.3
05:51:41.96 +28:18:24.7
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Aur-06-Q1b1x1_054643_TTUQ1b1x1_1787842_N2K9rk89/fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Aur-06-Q1b1x1_054643_TTUQ1b1x1_1787842_N2K9rk89/fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits
SExtractor catalog cache: saved Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits.cat to cache
SExtractor catalog cache: saved Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Aur-06-Q1b1x1_054643_TTUQ1b1x1_1787842_N2K9rk89/fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Aur-06-Q1b1x1_054643_TTUQ1b1x1_1787842_N2K9rk89/fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits
Creating symlink local_wcs_cache/wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits exists and is non-empty
wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits exists and is non-empty
wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits exists and is non-empty
wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits (1st reference image)
verification OK: wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits
Image size: 941.5'x626.9' 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: 06:00:00.480 +29:59:52.07 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-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits (1st new image)
verification OK: wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits
Image size: 944.6'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:59:51.679 +30:03:49.56 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 06:00:00.480 +29:59:52.07
Second-epoch image center 05:59:51.679 +30:03:49.56
Angular distance between the image centers 0.0732 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits (2nd new image)
verification OK: wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits
Image size: 944.5'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:59:54.014 +30:03:58.51 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 06:00:00.480 +29:59:52.07
Second-epoch image center 05:59:54.014 +30:03:58.51
Angular distance between the image centers 0.0723 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 05:59:51.679 +30:03:49.56
Second-epoch second image center 05:59:54.014 +30:03:58.51
Angular distance between the image centers 0.00878 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-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits &> /tmp/tmp.xDa0u2HPQ8
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits &> /tmp/tmp.cvu1EfXgPx
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Aur-06-Q1b1x1_054643_TTUQ1b1x1_1787842_N2K9rk89/fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits &> /tmp/tmp.9ShlaLGlsl
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Aur-06-Q1b1x1_054643_TTUQ1b1x1_1787842_N2K9rk89/fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Aur-06-Q1b1x1_054643_TTUQ1b1x1_1787842_N2K9rk89/fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits &> /tmp/tmp.Oywr2s5jCf
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Aur-06-Q1b1x1_054643_TTUQ1b1x1_1787842_N2K9rk89/fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.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-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits and wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.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-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits and wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits.wcscat
Found non-empty wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits and wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits.wcscat
The reference image (wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits) and catalog (wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits.wcscat) found
'wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits.wcscat' -> 'wcsmag.cat'
Read 212828 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 80.5608 to 99.6889 deg, Dec +24.3185 to +35.3069 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 80.5608 to 99.6889 deg, Dec 24.3185 to 35.3069 deg
Loaded 17188 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): 9142 out of 14161 total matches.
Matched with Tycho-2 14161 out of 212828 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.790850
a=0.000000 b=1.000000 c=22.790850
From vast_summary.log: estimated ref. image limiting mag.: -7.36
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.43
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.43
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 212828 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 80.5608 to 99.6889 deg, Dec +24.3185 to +35.3069 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 80.5608 to 99.6889 deg, Dec 24.3185 to 35.3069 deg
Loaded 17188 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): 9142 out of 14161 total matches.
Matched with Tycho-2 14161 out of 212828 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits:
Forced-photometry filter: calibrated wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits -> calib.txt_param_ref_wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits (aperture=4.5)
Read 212641 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 80.5698 to 99.6891 deg, Dec +24.3258 to +35.3145 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 80.5698 to 99.6891 deg, Dec 24.3258 to 35.3145 deg
Loaded 17176 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): 9258 out of 14259 total matches.
Matched with Tycho-2 14259 out of 212641 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits:
Forced-photometry filter: calibrated wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits -> calib.txt_param_ref_wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits (aperture=4.5)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 105 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
1.9 pix Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits
1.9 pix Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits
3.2 pix fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits
3.2 pix fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits
1.9 pix wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits
1.9 pix wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits
Limiting magnitude estimates:
15.4 mag. Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits
15.4 mag. Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits
13.1 mag. fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits
13.1 mag. fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits
All-image limiting magnitude estimate: 13.1 (SNR ) 12.6 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.xDa0u2HPQ8 (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_2026-07-22_CI_Aur-06-Q1b1x1_054643_TTUQ1b1x1_1787842_N2K9rk89/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.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-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits' -> 'wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits
WCS_IMAGE_NAME=wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits
WCS-calibrated image found: wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits
Checking if the catalog wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits.wcscat corresponding to the image wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits alredy exist and is non-empty...
Catalog wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits.wcscat corresponding to the image wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits
WCS catalog name: wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.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=79, blended=32424, bad_region=1, passed=212748
Got 212748 stars (including 179989 good ones) from the SExtractor catalog wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits.wcscat
util/solve_plate_with_UCAC5 got 212748 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 908 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 206492 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 206490 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 206492 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 928 stars left (next iteration limit 1020)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits N_match=928 sigma_overall_arcsec=0.485 sigma_q1_arcsec=0.526 sigma_q2_arcsec=0.439 sigma_q3_arcsec=0.490 sigma_q4_arcsec=0.462 n_q1=199 n_q2=266 n_q3=222 n_q4=241 worst_quadrant_to_overall_ratio=1.084
The image catalog is written to wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits -region wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.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.cvu1EfXgPx (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_2026-07-22_CI_Aur-06-Q1b1x1_054643_TTUQ1b1x1_1787842_N2K9rk89/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.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-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits' -> 'wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits
WCS_IMAGE_NAME=wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits
WCS-calibrated image found: wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits
Checking if the catalog wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits.wcscat corresponding to the image wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits alredy exist and is non-empty...
Catalog wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits.wcscat corresponding to the image wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits
WCS catalog name: wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.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=51, blended=32176, bad_region=4, passed=212590
Got 212590 stars (including 180083 good ones) from the SExtractor catalog wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits.wcscat
util/solve_plate_with_UCAC5 got 212590 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 926 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 207885 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 207885 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 207884 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 936 stars left (next iteration limit 1029)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits N_match=936 sigma_overall_arcsec=0.466 sigma_q1_arcsec=0.582 sigma_q2_arcsec=0.427 sigma_q3_arcsec=0.512 sigma_q4_arcsec=0.420 n_q1=198 n_q2=272 n_q3=210 n_q4=256 worst_quadrant_to_overall_ratio=1.248
The image catalog is written to wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits -region wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.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.9ShlaLGlsl (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_2026-07-22_CI_Aur-06-Q1b1x1_054643_TTUQ1b1x1_1787842_N2K9rk89/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Aur-06-Q1b1x1_054643_TTUQ1b1x1_1787842_N2K9rk89/fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Aur-06-Q1b1x1_054643_TTUQ1b1x1_1787842_N2K9rk89/fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Aur-06-Q1b1x1_054643_TTUQ1b1x1_1787842_N2K9rk89/fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Aur-06-Q1b1x1_054643_TTUQ1b1x1_1787842_N2K9rk89/fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Aur-06-Q1b1x1_054643_TTUQ1b1x1_1787842_N2K9rk89/fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.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_2026-07-22_CI_Aur-06-Q1b1x1_054643_TTUQ1b1x1_1787842_N2K9rk89/fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits
WCS_IMAGE_NAME=wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits
WCS-calibrated image found: wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits
Checking if the catalog wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits.wcscat corresponding to the image wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits.wcscat corresponding to the image wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Aur-06-Q1b1x1_054643_TTUQ1b1x1_1787842_N2K9rk89/fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits
WCS catalog name: wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=1768, bad_region=0, passed=36294
Got 36294 stars (including 34488 good ones) from the SExtractor catalog wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits.wcscat
util/solve_plate_with_UCAC5 got 36294 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 944.6'
Seting catalog search parameters based on the expected field of view 944.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013119 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010496 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 629 (Dec 24.1 to 35.5)
Done reading UCAC5 zone files...
Matched 926 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 921 matched stars entering correct_measured_positions(), 888 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 921 matched stars entering correct_measured_positions(), 35327 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 629 (Dec 24.1 to 35.5)
Done reading UCAC5 zone files...
Matched 925 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 920 matched stars entering correct_measured_positions(), 35326 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Accuracy estimation diagnostic: 920 matched stars entering correct_measured_positions(), 35324 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 920 stars left (next iteration limit 1013)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits N_match=920 sigma_overall_arcsec=0.472 sigma_q1_arcsec=0.493 sigma_q2_arcsec=0.641 sigma_q3_arcsec=0.384 sigma_q4_arcsec=0.488 n_q1=248 n_q2=155 n_q3=336 n_q4=181 worst_quadrant_to_overall_ratio=1.357
The image catalog is written to wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Aur-06-Q1b1x1_054643_TTUQ1b1x1_1787842_N2K9rk89/fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits -region wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.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.Oywr2s5jCf (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_2026-07-22_CI_Aur-06-Q1b1x1_054643_TTUQ1b1x1_1787842_N2K9rk89/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Aur-06-Q1b1x1_054643_TTUQ1b1x1_1787842_N2K9rk89/fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Aur-06-Q1b1x1_054643_TTUQ1b1x1_1787842_N2K9rk89/fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Aur-06-Q1b1x1_054643_TTUQ1b1x1_1787842_N2K9rk89/fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Aur-06-Q1b1x1_054643_TTUQ1b1x1_1787842_N2K9rk89/fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Aur-06-Q1b1x1_054643_TTUQ1b1x1_1787842_N2K9rk89/fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.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_2026-07-22_CI_Aur-06-Q1b1x1_054643_TTUQ1b1x1_1787842_N2K9rk89/fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits
WCS_IMAGE_NAME=wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits
WCS-calibrated image found: wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits
Checking if the catalog wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits.wcscat corresponding to the image wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits.wcscat corresponding to the image wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Aur-06-Q1b1x1_054643_TTUQ1b1x1_1787842_N2K9rk89/fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits
WCS catalog name: wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.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=3, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=1507, bad_region=0, passed=34711
Got 34711 stars (including 33168 good ones) from the SExtractor catalog wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits.wcscat
util/solve_plate_with_UCAC5 got 34711 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 944.5'
Seting catalog search parameters based on the expected field of view 944.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013118 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010494 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 629 (Dec 24.1 to 35.5)
Done reading UCAC5 zone files...
Matched 926 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 922 matched stars entering correct_measured_positions(), 885 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 922 matched stars entering correct_measured_positions(), 33736 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 629 (Dec 24.1 to 35.5)
Done reading UCAC5 zone files...
Matched 926 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 921 matched stars entering correct_measured_positions(), 33743 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Accuracy estimation diagnostic: 921 matched stars entering correct_measured_positions(), 33742 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 921 stars left (next iteration limit 1014)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits N_match=921 sigma_overall_arcsec=0.480 sigma_q1_arcsec=0.486 sigma_q2_arcsec=0.633 sigma_q3_arcsec=0.442 sigma_q4_arcsec=0.501 n_q1=245 n_q2=151 n_q3=341 n_q4=184 worst_quadrant_to_overall_ratio=1.320
The image catalog is written to wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Aur-06-Q1b1x1_054643_TTUQ1b1x1_1787842_N2K9rk89/fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits -region wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Aur-06-Q1b1x1_054643_TTUQ1b1x1_1787842_N2K9rk89/wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-45-20_20.00sec_-0.00C_LIGHTs_0424.fits
Saving fully-calibrated image wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Aur-06-Q1b1x1_054643_TTUQ1b1x1_1787842_N2K9rk89/wcs_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425.fits
Preparing the HTML report for the field Aur-06-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 05:27:29.87 +29:01:21.7: 12.13 +/- 0.01 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 06:01:03.30 +30:08:34.2: 12.26 +/- 0.01 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 05:36:11.44 +31:54:35.4: 12.61 +/- 0.02 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 06:07:00.15 +25:02:24.9: 12.26 +/- 0.01 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 05:27:12.68 +34:01:23.4: 12.58 +/- 0.02 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 05:52:47.41 +34:43:58.7: 12.66 +/- 0.02 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 06:07:00.15 +25:02:24.9: 12.06 +/- 0.01 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 05:27:12.68 +34:01:23.4: 12.63 +/- 0.02 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 05:36:11.44 +31:54:35.4: 12.67 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.15 +/- 0.01
Forced photometry filter REJECTED candidate at 06:07:00.15 +25:02:24.9: ref_mag=12.15 +/- 0.01 new_mean_mag=11.4973 delta=0.65 (need > 0.90)
Forced photometry reference-image weighted average: 12.64 +/- 0.01
Forced photometry filter REJECTED candidate at 05:36:11.44 +31:54:35.4: ref_mag=12.64 +/- 0.01 new_mean_mag=12.6960 delta=-0.06 (need > 0.90)
Forced photometry reference-image weighted average: 12.61 +/- 0.01
Forced photometry filter REJECTED candidate at 05:27:12.68 +34:01:23.4: ref_mag=12.61 +/- 0.01 new_mean_mag=12.6682 delta=-0.06 (need > 0.90)
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 05:27:29.87 +29:01:21.7: 12.13 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.13 +/- 0.01
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 05:52:47.41 +34:43:58.7: 12.65 +/- 0.02 detection
Forced photometry filter REJECTED candidate at 05:27:29.87 +29:01:21.7: ref_mag=12.13 +/- 0.01 new_mean_mag=12.1185 delta=0.01 (need > 0.90)
Forced photometry reference-image weighted average: 12.66 +/- 0.01
Forced photometry filter REJECTED candidate at 05:52:47.41 +34:43:58.7: ref_mag=12.66 +/- 0.01 new_mean_mag=12.6149 delta=0.04 (need > 0.90)
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 06:01:03.30 +30:08:34.2: 12.27 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.27 +/- 0.01
Forced photometry filter REJECTED candidate at 06:01:03.30 +30:08:34.2: ref_mag=12.27 +/- 0.01 new_mean_mag=12.1729 delta=0.09 (need > 0.90)
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 05:50:51.54 +33:33:39.2: 16.13 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 05:50:51.54 +33:33:39.2: 16.11 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 05:40:56.89 +28:06:34.2: 12.34 +/- 0.02 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 05:38:47.97 +35:04:24.0: 12.88 +/- 0.03 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 05:39:20.82 +30:53:54.8: 12.82 +/- 0.03 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 05:40:56.89 +28:06:34.2: 12.31 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.33 +/- 0.01
Forced photometry filter REJECTED candidate at 05:40:56.89 +28:06:34.2: ref_mag=12.33 +/- 0.01 new_mean_mag=12.2318 delta=0.09 (need > 0.90)
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 05:38:47.97 +35:04:24.0: 12.95 +/- 0.03 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 05:39:20.82 +30:53:54.8: 12.85 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.02
Forced photometry filter REJECTED candidate at 05:38:47.97 +35:04:24.0: ref_mag=12.91 +/- 0.02 new_mean_mag=12.8206 delta=0.09 (need > 0.90)
Forced photometry reference-image weighted average: 12.84 +/- 0.02
Forced photometry filter REJECTED candidate at 05:39:20.82 +30:53:54.8: ref_mag=12.84 +/- 0.02 new_mean_mag=12.5920 delta=0.24 (need > 0.90)
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 05:59:47.26 +26:45:31.7: 12.28 +/- 0.01 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 05:59:47.26 +26:45:31.7: 12.24 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.26 +/- 0.01
Forced photometry filter KEPT candidate at 05:59:47.26 +26:45:31.7: ref_mag=12.26 +/- 0.01 new_mean_mag=11.1954 delta=1.07 (need > 0.90)
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 06:17:05.51 +28:56:03.3: 12.73 +/- 0.02 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 06:03:26.73 +31:46:01.4: 11.79 +/- 0.01 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 06:09:20.04 +26:31:43.3: 10.13 +/- 0.00 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 06:09:20.04 +26:31:43.3: 10.12 +/- 0.00 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 06:17:05.51 +28:56:03.3: 12.81 +/- 0.02 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 06:03:26.73 +31:46:01.4: 11.77 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.01
Forced photometry reference-image weighted average: 10.13 +/- 0.00
Forced photometry filter KEPT candidate at 06:17:05.51 +28:56:03.3: ref_mag=12.77 +/- 0.01 new_mean_mag=11.8422 delta=0.93 (need > 0.90)
Forced photometry reference-image weighted average: 11.78 +/- 0.01
Forced photometry filter KEPT candidate at 06:09:20.04 +26:31:43.3: ref_mag=10.13 +/- 0.00 new_mean_mag=9.1655 delta=0.96 (need > 0.90)
Forced photometry filter KEPT candidate at 06:03:26.73 +31:46:01.4: ref_mag=11.78 +/- 0.01 new_mean_mag=10.8162 delta=0.96 (need > 0.90)
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 06:08:09.46 +31:08:02.6: 13.18 +/- 0.02 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 06:25:39.14 +31:50:16.1: 12.97 +/- 0.02 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 06:08:45.08 +25:51:18.7: 11.37 +/- 0.01 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 06:08:09.46 +31:08:02.6: 13.22 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.02
Forced photometry filter KEPT candidate at 06:08:09.46 +31:08:02.6: ref_mag=13.20 +/- 0.02 new_mean_mag=12.2101 delta=0.99 (need > 0.90)
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 06:01:22.02 +28:33:04.1: 12.62 +/- 0.02 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 06:25:39.14 +31:50:16.1: 12.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.01
Forced photometry filter KEPT candidate at 06:25:39.14 +31:50:16.1: ref_mag=12.97 +/- 0.01 new_mean_mag=11.9304 delta=1.04 (need > 0.90)
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 06:08:45.08 +25:51:18.7: 11.37 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.37 +/- 0.00
Forced photometry filter KEPT candidate at 06:08:45.08 +25:51:18.7: ref_mag=11.37 +/- 0.00 new_mean_mag=10.3892 delta=0.98 (need > 0.90)
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 06:01:22.02 +28:33:04.1: 12.61 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.01
Forced photometry filter KEPT candidate at 06:01:22.02 +28:33:04.1: ref_mag=12.61 +/- 0.01 new_mean_mag=11.6785 delta=0.94 (need > 0.90)
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 06:08:59.52 +27:55:02.2: 12.17 +/- 0.01 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 06:08:59.52 +27:55:02.2: 12.16 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.17 +/- 0.01
Forced photometry filter KEPT candidate at 06:08:59.52 +27:55:02.2: ref_mag=12.17 +/- 0.01 new_mean_mag=11.2309 delta=0.94 (need > 0.90)
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 05:33:49.91 +26:38:06.4: 11.27 +/- 0.01 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 05:33:49.91 +26:38:06.4: 11.27 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.27 +/- 0.00
Forced photometry filter KEPT candidate at 05:33:49.91 +26:38:06.4: ref_mag=11.27 +/- 0.00 new_mean_mag=10.2730 delta=0.99 (need > 0.90)
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 06:07:04.47 +25:40:36.7: 12.58 +/- 0.02 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 06:07:04.47 +25:40:36.7: 12.54 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.56 +/- 0.01
Forced photometry filter KEPT candidate at 06:07:04.47 +25:40:36.7: ref_mag=12.56 +/- 0.01 new_mean_mag=11.6543 delta=0.90 (need > 0.90)
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 05:49:34.61 +27:15:26.4: 13.16 +/- 0.03 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 05:49:48.92 +25:25:25.0: 11.97 +/- 0.01 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 05:44:22.61 +31:10:31.9: 14.74 +/- 0.11 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 05:49:34.61 +27:15:26.4: 13.11 +/- 0.03 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 05:49:48.92 +25:25:25.0: 11.90 +/- 0.01 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Forced photometry filter KEPT candidate at 05:49:34.61 +27:15:26.4: ref_mag=13.14 +/- 0.02 new_mean_mag=12.0962 delta=1.04 (need > 0.90)
Forced photometry reference-image weighted average: 11.93 +/- 0.01
Forced photometry filter KEPT candidate at 05:49:48.92 +25:25:25.0: ref_mag=11.93 +/- 0.01 new_mean_mag=10.8551 delta=1.08 (need > 0.90)
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 05:44:22.61 +31:10:31.9: 14.57 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.64 +/- 0.07
Forced photometry filter KEPT candidate at 05:44:22.61 +31:10:31.9: ref_mag=14.64 +/- 0.07 new_mean_mag=12.3680 delta=2.27 (need > 0.90)
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 06:09:43.38 +25:12:22.8: 12.84 +/- 0.02 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 05:50:37.25 +31:42:40.4: 13.97 +/- 0.05 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 06:09:43.38 +25:12:22.8: 12.84 +/- 0.02 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 05:50:37.25 +31:42:40.4: 13.96 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.01
Forced photometry reference-image weighted average: 13.97 +/- 0.04
Forced photometry filter KEPT candidate at 06:09:43.38 +25:12:22.8: ref_mag=12.84 +/- 0.01 new_mean_mag=11.8205 delta=1.02 (need > 0.90)
Forced photometry filter KEPT candidate at 05:50:37.25 +31:42:40.4: ref_mag=13.97 +/- 0.04 new_mean_mag=12.7137 delta=1.25 (need > 0.90)
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 05:59:02.03 +32:58:47.1: 12.42 +/- 0.01 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 05:59:02.03 +32:58:47.1: 12.40 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.41 +/- 0.01
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 06:01:25.27 +33:26:00.4: 13.50 +/- 0.04 detection
Forced photometry filter KEPT candidate at 05:59:02.03 +32:58:47.1: ref_mag=12.41 +/- 0.01 new_mean_mag=11.3865 delta=1.02 (need > 0.90)
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 05:48:40.17 +26:28:28.7: 12.39 +/- 0.01 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 06:01:25.27 +33:26:00.4: 13.44 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.02
Forced photometry filter KEPT candidate at 06:01:25.27 +33:26:00.4: ref_mag=13.47 +/- 0.02 new_mean_mag=12.3135 delta=1.16 (need > 0.90)
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 05:48:40.17 +26:28:28.7: 12.37 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.38 +/- 0.01
Forced photometry filter KEPT candidate at 05:48:40.17 +26:28:28.7: ref_mag=12.38 +/- 0.01 new_mean_mag=11.3629 delta=1.02 (need > 0.90)
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 06:30:54.31 +27:45:39.4: 12.30 +/- 0.01 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 06:02:50.44 +34:41:47.7: 14.13 +/- 0.06 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 05:57:39.56 +27:33:47.9: 13.02 +/- 0.02 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 06:02:50.44 +34:41:47.7: 13.95 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.03 +/- 0.04
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 06:30:54.31 +27:45:39.4: 12.32 +/- 0.01 detection
Forced photometry filter KEPT candidate at 06:02:50.44 +34:41:47.7: ref_mag=14.03 +/- 0.04 new_mean_mag=12.8159 delta=1.21 (need > 0.90)
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 05:57:39.56 +27:33:47.9: 13.04 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.31 +/- 0.01
Forced photometry filter KEPT candidate at 06:30:54.31 +27:45:39.4: ref_mag=12.31 +/- 0.01 new_mean_mag=11.2620 delta=1.05 (need > 0.90)
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 06:10:18.22 +32:03:09.6: 12.72 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.02
Forced photometry filter KEPT candidate at 05:57:39.56 +27:33:47.9: ref_mag=13.03 +/- 0.02 new_mean_mag=11.9597 delta=1.07 (need > 0.90)
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 06:10:18.22 +32:03:09.6: 12.72 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.72 +/- 0.01
Forced photometry filter KEPT candidate at 06:10:18.22 +32:03:09.6: ref_mag=12.72 +/- 0.01 new_mean_mag=11.7626 delta=0.96 (need > 0.90)
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 06:19:09.17 +32:18:41.0: 11.58 +/- 0.01 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 06:19:09.17 +32:18:41.0: 11.59 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.59 +/- 0.00
Forced photometry filter KEPT candidate at 06:19:09.17 +32:18:41.0: ref_mag=11.59 +/- 0.00 new_mean_mag=10.6135 delta=0.97 (need > 0.90)
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 05:52:52.97 +29:50:15.6: 12.23 +/- 0.01 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 06:15:37.37 +29:27:29.3: 13.48 +/- 0.04 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 05:44:31.11 +30:40:39.2: 11.45 +/- 0.01 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 06:15:37.37 +29:27:29.3: 13.44 +/- 0.04 detection
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 05:52:52.97 +29:50:15.6: 12.21 +/- 0.01 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.03
Forced photometry reference-image weighted average: 12.22 +/- 0.01
Forced photometry filter KEPT candidate at 06:15:37.37 +29:27:29.3: ref_mag=13.46 +/- 0.03 new_mean_mag=12.2226 delta=1.24 (need > 0.90)
Forced photometry filter KEPT candidate at 05:52:52.97 +29:50:15.6: ref_mag=12.22 +/- 0.01 new_mean_mag=11.3017 delta=0.92 (need > 0.90)
Forced photometry on wcs_Aur-06-Q1b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 05:44:31.11 +30:40:39.2: 11.43 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.44 +/- 0.00
Forced photometry filter KEPT candidate at 05:44:31.11 +30:40:39.2: ref_mag=11.44 +/- 0.00 new_mean_mag=10.4463 delta=0.99 (need > 0.90)
Adding exclusion_list_local.txt__out09876.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out109191.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out113818.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out124884.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136086.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out145768.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out149793.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out157556.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out162899.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out169250.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out173004.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out183260.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out186034.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out186660.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189546.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out198853.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out210727.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out242461.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34292.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44640.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55107.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out61697.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out62099.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out69618.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out70434.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out80981.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out81129.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out92254.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 24s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 22s
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Considering the candidate 242158_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 242158_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
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Considering the candidate 242161_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 242161_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
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Considering the candidate 242162_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 242162_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
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Considering the candidate 242163_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 242163_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
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Considering the candidate 242164_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 242164_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 05:38:59.57 +34:57:14.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 242165_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 242165_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 05:46:35.52 +33:48:09.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 242170_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 242170_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 05:51:20.40 +32:13:24.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 242178_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 242178_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
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Considering the candidate 242179_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 242179_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
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Considering the candidate 242183_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 242183_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 05:52:15.15 +32:30:34.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 242184_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 242184_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 05:52:19.76 +32:31:53.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 242185_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 242185_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 05:52:17.92 +32:31:19.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 242349_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 242349_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 05:42:12.25 +32:03:12.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 242372_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 242372_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 05:27:41.44 +34:26:42.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 242443_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 242443_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 05:52:16.40 +32:35:30.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 242459_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 242459_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 06:09:27.74 +28:29:43.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 242461_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
Preparing report for the candidate 242461_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
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Considering the candidate 242501_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 242501_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 05:31:20.48 +35:01:42.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 242525_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 242525_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 05:51:00.38 +27:56:29.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 242558_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 242558_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 06:09:09.86 +34:55:01.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 242571_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 242571_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 05:26:33.28 +28:37:18.4 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 242574_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 242574_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 05:26:40.64 +34:23:17.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 242607_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 242607_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 06:00:52.46 +27:35:09.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 242620_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 242620_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 05:30:34.09 +33:00:21.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 242630_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 242630_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 05:25:17.75 +30:10:45.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 242711_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 242711_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
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Considering the candidate 242726_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 242726_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 05:37:15.16 +34:48:40.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 242782_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 242782_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 05:40:55.04 +32:52:27.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 242808_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 242808_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 05:38:32.65 +30:30:47.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 242838_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 242838_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
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Considering the candidate 242857_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 242857_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 05:47:19.27 +31:39:29.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 242861_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 242861_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
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Considering the candidate 242966_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 242966_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 167626_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 167626_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 05:57:59.66 +25:57:18.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 116475_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 116475_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 06:15:22.21 +29:29:44.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 159674_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 159674_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 05:53:19.86 +27:36:46.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 117937_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 117937_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 06:06:22.33 +29:30:43.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 82530_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 82530_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 06:21:56.71 +30:53:14.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 189546_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
Preparing report for the candidate 189546_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
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Considering the candidate 168593_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 168593_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 06:06:18.11 +25:36:47.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 124884_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
Preparing report for the candidate 124884_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
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Considering the candidate 186034_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
Preparing report for the candidate 186034_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
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Considering the candidate 69618_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
Preparing report for the candidate 69618_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
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Considering the candidate 136018_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 136018_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 05:54:21.07 +28:36:31.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 144103_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 144103_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 05:51:41.97 +28:18:24.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 20812_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 20812_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 06:33:11.35 +33:40:07.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 24946_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 24946_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 05:43:37.02 +33:54:12.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 81129_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
Preparing report for the candidate 81129_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
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Considering the candidate 62099_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
Preparing report for the candidate 62099_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
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Considering the candidate 136086_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
Preparing report for the candidate 136086_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
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Considering the candidate 107520_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 107520_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 06:04:28.70 +29:51:03.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 173004_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
Preparing report for the candidate 173004_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
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Considering the candidate 123168_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 123168_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 05:59:32.78 +29:09:40.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 149793_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
Preparing report for the candidate 149793_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
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Considering the candidate 125198_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 125198_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 05:36:52.15 +29:02:14.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 186660_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
Preparing report for the candidate 186660_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
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Considering the candidate 79040_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 79040_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 06:29:12.80 +30:56:48.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56703_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 56703_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 05:57:14.78 +32:22:38.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 137469_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 137469_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 06:04:17.02 +28:29:01.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 63229_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 63229_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 05:48:03.10 +32:03:18.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 87651_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 87651_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 06:26:42.38 +30:33:43.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169250_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
Preparing report for the candidate 169250_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
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Considering the candidate 146773_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 146773_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 05:30:39.90 +28:00:49.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 99439_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 99439_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 06:10:54.78 +30:13:49.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 28054_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 28054_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
Rejecting candidate due to large distance (30.6") between the two second-epoch detections
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Considering the candidate 162899_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
Preparing report for the candidate 162899_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
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Considering the candidate 198853_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
Preparing report for the candidate 198853_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
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Considering the candidate 79766_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 79766_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 06:20:38.32 +31:03:04.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 80981_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
Preparing report for the candidate 80981_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
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Considering the candidate 14794_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 14794_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 05:38:03.97 +34:25:02.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 66618_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 66618_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 05:59:31.51 +31:56:02.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 156560_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 156560_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 05:40:49.22 +27:36:15.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 104428_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 104428_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 05:37:46.36 +30:03:47.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 153284_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 153284_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 05:54:15.16 +27:47:45.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 75870_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 75870_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 06:10:30.94 +31:25:48.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 135068_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 135068_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 05:59:21.06 +28:36:16.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 64657_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 64657_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 06:33:17.02 +31:35:29.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 93431_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 93431_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 06:22:50.07 +30:19:51.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 210727_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
Preparing report for the candidate 210727_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 70434_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
Preparing report for the candidate 70434_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167008_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 167008_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 06:17:33.75 +25:26:43.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 108247_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 108247_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 05:39:04.38 +29:55:34.6 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11759_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 11759_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 05:41:51.67 +34:35:22.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 59148_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 59148_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 06:07:00.35 +32:13:10.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 44640_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
Preparing report for the candidate 44640_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 28544_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 28544_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 05:48:23.52 +33:45:02.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34292_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
Preparing report for the candidate 34292_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 183260_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
Preparing report for the candidate 183260_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 209789_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 209789_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 05:50:00.52 +25:17:11.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62401_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 62401_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 06:08:39.99 +32:01:54.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 158400_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 158400_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 06:15:28.42 +27:23:45.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 145768_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
Preparing report for the candidate 145768_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09876_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
Preparing report for the candidate 09876_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 157556_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
Preparing report for the candidate 157556_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 88249_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 88249_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 05:56:48.34 +30:50:08.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 61697_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
Preparing report for the candidate 61697_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 77282_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 77282_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 06:09:57.73 +31:24:25.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 153136_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 153136_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 06:28:29.25 +27:29:07.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 55107_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
Preparing report for the candidate 55107_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115105_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 115105_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 05:49:47.46 +29:32:53.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 109191_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
Preparing report for the candidate 109191_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39563_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 39563_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 06:17:14.28 +33:12:22.0 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113818_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
Preparing report for the candidate 113818_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159325_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
The candidate 159325_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425 did not pass the final checks
**** FOUND 06:01:00.44 +27:34:22.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 92254_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
Preparing report for the candidate 92254_fd_Aur-06-Q1b1x1_2026-07-22_05-46-11_20.00sec_-0.00C_LIGHTs_0425
make_report_in_HTML.sh Phase 2 (HTML assembly): 4s
make_report_in_HTML.sh TOTAL: 50s
Prepared the HTML report for the field Aur-06-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
05:39:04.35 +29:55:34.3
05:51:41.96 +28:18:24.7
06:02:50.44 +34:41:47.7
05:52:52.97 +29:50:15.6
06:15:37.37 +29:27:29.3
06:17:05.51 +28:56:03.3
06:01:22.02 +28:33:04.1
06:30:54.31 +27:45:39.4
06:08:59.52 +27:55:02.2
05:57:39.56 +27:33:47.9
05:49:48.92 +25:25:25.0
06:07:04.47 +25:40:36.7
06:08:45.08 +25:51:18.7
05:48:40.17 +26:28:28.7
06:09:20.04 +26:31:43.3
05:33:49.91 +26:38:06.4
05:59:47.26 +26:45:31.7
05:49:34.61 +27:15:26.4
06:09:43.38 +25:12:22.8
05:50:51.54 +33:33:39.2
06:01:25.27 +33:26:00.4
05:59:02.03 +32:58:47.1
06:19:09.17 +32:18:41.0
06:10:18.22 +32:03:09.6
06:25:39.14 +31:50:16.1
06:03:26.73 +31:46:01.4
05:50:37.25 +31:42:40.4
05:44:22.61 +31:10:31.9
06:08:09.46 +31:08:02.6
05:44:31.11 +30:40:39.2
########### Completed Aur-06-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 ####
05:39:04.35 +29:55:34.3
05:51:41.96 +28:18:24.7
05:50:51.54 +33:33:39.2
05:59:47.26 +26:45:31.7
06:17:05.51 +28:56:03.3
06:09:20.04 +26:31:43.3
06:03:26.73 +31:46:01.4
06:08:09.46 +31:08:02.6
06:25:39.14 +31:50:16.1
06:01:22.02 +28:33:04.1
06:08:45.08 +25:51:18.7
06:08:59.52 +27:55:02.2
05:33:49.91 +26:38:06.4
06:07:04.47 +25:40:36.7
05:49:48.92 +25:25:25.0
05:49:34.61 +27:15:26.4
05:44:22.61 +31:10:31.9
06:09:43.38 +25:12:22.8
05:50:37.25 +31:42:40.4
05:59:02.03 +32:58:47.1
06:01:25.27 +33:26:00.4
05:48:40.17 +26:28:28.7
06:30:54.31 +27:45:39.4
06:02:50.44 +34:41:47.7
05:57:39.56 +27:33:47.9
06:10:18.22 +32:03:09.6
06:19:09.17 +32:18:41.0
05:52:52.97 +29:50:15.6
06:15:37.37 +29:27:29.3
05:44:31.11 +30:40:39.2
###################################################################################
05:39:04.35 +29:55:34.3 -- not an asteroid (will add it to exclusion list)
05:51:41.96 +28:18:24.7 -- not an asteroid (will add it to exclusion list)
05:50:51.54 +33:33:39.2 -- asteroid (will NOT add it to exclusion list)
05:59:47.26 +26:45:31.7 -- not an asteroid (will add it to exclusion list)
06:17:05.51 +28:56:03.3 -- not an asteroid (will add it to exclusion list)
06:09:20.04 +26:31:43.3 -- not an asteroid (will add it to exclusion list)
06:03:26.73 +31:46:01.4 -- not an asteroid (will add it to exclusion list)
06:08:09.46 +31:08:02.6 -- not an asteroid (will add it to exclusion list)
06:25:39.14 +31:50:16.1 -- not an asteroid (will add it to exclusion list)
06:01:22.02 +28:33:04.1 -- asteroid (will NOT add it to exclusion list)
06:08:45.08 +25:51:18.7 -- asteroid (will NOT add it to exclusion list)
06:08:59.52 +27:55:02.2 -- not an asteroid (will add it to exclusion list)
05:33:49.91 +26:38:06.4 -- not an asteroid (will add it to exclusion list)
06:07:04.47 +25:40:36.7 -- not an asteroid (will add it to exclusion list)
05:49:48.92 +25:25:25.0 -- not an asteroid (will add it to exclusion list)
05:49:34.61 +27:15:26.4 -- not an asteroid (will add it to exclusion list)
05:44:22.61 +31:10:31.9 -- asteroid (will NOT add it to exclusion list)
06:09:43.38 +25:12:22.8 -- not an asteroid (will add it to exclusion list)
05:50:37.25 +31:42:40.4 -- not an asteroid (will add it to exclusion list)
05:59:02.03 +32:58:47.1 -- not an asteroid (will add it to exclusion list)
06:01:25.27 +33:26:00.4 -- not an asteroid (will add it to exclusion list)
05:48:40.17 +26:28:28.7 -- asteroid (will NOT add it to exclusion list)
06:30:54.31 +27:45:39.4 -- not an asteroid (will add it to exclusion list)
06:02:50.44 +34:41:47.7 -- not an asteroid (will add it to exclusion list)
05:57:39.56 +27:33:47.9 -- not an asteroid (will add it to exclusion list)
06:10:18.22 +32:03:09.6 -- not an asteroid (will add it to exclusion list)
06:19:09.17 +32:18:41.0 -- not an asteroid (will add it to exclusion list)
05:52:52.97 +29:50:15.6 -- not an asteroid (will add it to exclusion list)
06:15:37.37 +29:27:29.3 -- not an asteroid (will add it to exclusion list)
05:44:31.11 +30:40:39.2 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
05:33:49.91 +26:38:06.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:39:04.35 +29:55:34.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:44:31.11 +30:40:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:34.61 +27:15:26.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:48.92 +25:25:25.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:37.25 +31:42:40.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:41.96 +28:18:24.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:52.97 +29:50:15.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:39.56 +27:33:47.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:59:02.03 +32:58:47.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:59:47.26 +26:45:31.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:25.27 +33:26:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:02:50.44 +34:41:47.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:03:26.73 +31:46:01.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:07:04.47 +25:40:36.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:08:09.46 +31:08:02.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:08:59.52 +27:55:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:09:20.04 +26:31:43.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:09:43.38 +25:12:22.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:10:18.22 +32:03:09.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:15:37.37 +29:27:29.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:17:05.51 +28:56:03.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:19:09.17 +32:18:41.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:25:39.14 +31:50:16.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:30:54.31 +27:45:39.4 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
05:33:49.91 +26:38:06.4 -- a known variable star
05:39:04.35 +29:55:34.3 -- a known variable star
05:44:31.11 +30:40:39.2 -- a known variable star
05:49:34.61 +27:15:26.4 -- a known variable star
05:49:48.92 +25:25:25.0 -- a known variable star
05:50:37.25 +31:42:40.4 -- a known variable star
05:51:41.96 +28:18:24.7 -- a known variable star
05:52:52.97 +29:50:15.6 -- a known variable star
05:57:39.56 +27:33:47.9 -- a known variable star
05:59:02.03 +32:58:47.1 -- a known variable star
05:59:47.26 +26:45:31.7 -- a known variable star
06:01:25.27 +33:26:00.4 -- a known variable star
06:02:50.44 +34:41:47.7 -- a known variable star
06:03:26.73 +31:46:01.4 -- a known variable star
06:07:04.47 +25:40:36.7 -- a known variable star
06:08:09.46 +31:08:02.6 -- a known variable star
06:08:59.52 +27:55:02.2 -- a known variable star
06:09:20.04 +26:31:43.3 -- a known variable star
06:09:43.38 +25:12:22.8 -- a known variable star
06:10:18.22 +32:03:09.6 -- a known variable star
06:15:37.37 +29:27:29.3 -- a known variable star
06:17:05.51 +28:56:03.3 -- a known variable star
06:19:09.17 +32:18:41.0 -- a known variable star
06:25:39.14 +31:50:16.1 -- a known variable star
06:30:54.31 +27:45:39.4 -- a known variable star
Found 0 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
25 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
###################################################################################
exclusion_list_gaiadr2.txt NOT FOUND
exclusion_list_apass.txt NOT FOUND
IS_THIS_TEST_RUN= NO ALLOW_EXCLUSION_LIST_UPDATE= YES
#### Adding the following to the exclusion list ####
05:33:49.91 +26:38:06.4
05:39:04.35 +29:55:34.3
05:44:31.11 +30:40:39.2
05:49:34.61 +27:15:26.4
05:49:48.92 +25:25:25.0
05:50:37.25 +31:42:40.4
05:51:41.96 +28:18:24.7
05:52:52.97 +29:50:15.6
05:57:39.56 +27:33:47.9
05:59:02.03 +32:58:47.1
05:59:47.26 +26:45:31.7
06:01:25.27 +33:26:00.4
06:02:50.44 +34:41:47.7
06:03:26.73 +31:46:01.4
06:07:04.47 +25:40:36.7
06:08:09.46 +31:08:02.6
06:08:59.52 +27:55:02.2
06:09:20.04 +26:31:43.3
06:09:43.38 +25:12:22.8
06:10:18.22 +32:03:09.6
06:15:37.37 +29:27:29.3
06:17:05.51 +28:56:03.3
06:19:09.17 +32:18:41.0
06:25:39.14 +31:50:16.1
06:30:54.31 +27:45:39.4
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The observatory MPC code is V36
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Positions of planets computed with util/planet_finder/main.py for JD(UT)2461243.94826677 -observatory V36
07:07:28.79 +18:10:32.9 Mercury (2.5mag)
11:00:35.50 +07:07:07.4 Venus (-4.2mag)
05:00:00.87 +22:41:08.1 Mars (1.3mag)
08:27:42.32 +19:35:25.5 Jupiter (-1.8mag)
00:56:43.54 +03:22:18.4 Saturn (0.7mag)
04:09:23.16 +20:50:48.7 Uranus (5.8mag)
00:16:49.60 +00:18:43.2 Neptune (7.7mag)
20:29:46.16 -23:23:18.1 Pluto (14.4mag)
14:23:26.62 -19:51:40.5 Moon (-10.6mag)
-rw-r--r-- 1 apache apache 362 Jul 22 06:07 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461243.94826677:
08:27:43.26 +19:35:23.8 Io (6.0mag)
08:27:48.18 +19:35:02.1 Europa (6.3mag)
08:27:33.90 +19:36:02.7 Ganymede (5.6mag)
08:27:49.31 +19:35:03.0 Callisto (6.7mag)
08:25:43.47 +19:25:14.4 Himalia (15.7mag)
08:27:40.67 +19:35:32.8 Thebe (16.6mag)
08:25:05.66 +19:27:06.6 Elara (17.7mag)
08:31:34.09 +19:23:12.3 Pasiphae (17.9mag)
08:31:57.36 +19:42:24.7 Carme (19.0mag)
00:56:36.48 +03:22:45.1 Titan (8.5mag)
00:56:45.56 +03:22:24.9 Rhea (9.8mag)
00:56:12.40 +03:19:45.2 Iapetus (11.2mag)
00:56:44.00 +03:21:39.0 Hyperion (14.5mag)
00:56:28.07 +03:17:47.3 Phoebe (16.5mag)
-rw-r--r-- 1 apache apache 568 Jul 22 06:07 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461243.94826677:
18:07:40.08 -29:46:42.4 JWST
19:07:20.53 +04:25:39.6 Chandra
06:17:24.50 +24:09:53.8 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jul 22 06:07 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461243.94826677 -observatory V36
02:52:56.78 +15:47:25.4 17.8mag P/1996 R2 (Lagerkvist)
18:09:26.95 -34:36:04.5 13.8mag P/2010 H2 (Vales)
06:37:41.84 -68:22:54.5 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:04:52.45 +32:39:40.5 17.6mag C/2017 K2 (PANSTARRS)
02:45:59.92 +26:07:37.8 16.0mag P/2021 N1 (ZTF)
22:51:37.02 +32:08:40.4 17.3mag C/2022 E2 (ATLAS)
06:25:56.33 +26:47:46.6 16.7mag C/2022 N2 (PANSTARRS)
10:06:13.68 +29:14:00.4 16.9mag C/2022 QE78 (ATLAS)
09:17:38.98 +05:11:12.5 17.9mag C/2022 R6 (PANSTARRS)
15:11:00.01 -11:42:17.8 17.8mag P/2023 B1 (PANSTARRS)
21:33:40.68 +67:19:28.9 17.9mag C/2023 H5 (Lemmon)
16:09:19.34 -11:19:04.0 14.1mag C/2023 R1 (PANSTARRS)
08:22:14.35 +66:23:50.9 18.0mag C/2024 A1 (ATLAS)
07:48:16.22 +30:35:24.9 14.9mag C/2024 E1 (Wierzchos)
15:11:14.26 +15:33:28.6 17.6mag C/2024 G6 (ATLAS)
19:25:22.59 +41:26:29.8 13.7mag C/2024 J3 (ATLAS)
21:33:48.72 +47:39:40.0 17.7mag C/2024 R4 (PANSTARRS)
05:00:49.18 -13:19:40.9 15.6mag C/2024 T5 (ATLAS)
06:44:16.46 +27:02:35.1 17.9mag C/2025 J1 (Borisov)
07:22:13.82 -14:04:23.5 17.1mag C/2025 R3 (PANSTARRS)
10:10:40.92 +21:52:08.2 17.5mag C/2025 V2 (Rankin)
12:49:18.99 +03:21:32.9 17.0mag C/2025 Y1 (ATLAS)
16:21:53.86 +79:00:09.8 17.1mag C/2026 A2 (Bok)
02:57:39.26 +45:43:08.5 16.9mag C/2026 B2 (Sun-Gao)
11:33:44.62 +06:29:02.3 17.1mag A/2026 E1
21:37:09.02 -19:53:34.7 7.0mag 10P/Tempel
11:19:28.60 -02:27:06.3 16.2mag 29P/Schwassmann-Wachmann
04:17:15.77 +30:49:38.3 17.9mag 47P/Ashbrook-Jackson
10:33:14.67 +10:07:13.6 17.1mag 63P/Wild
00:52:34.34 -05:04:00.5 15.5mag 65P/Gunn
04:56:27.87 +20:38:49.8 13.7mag 78P/Gehrels
02:40:39.94 +12:07:56.9 16.4mag 88P/Howell
07:10:43.61 +29:36:45.4 15.9mag 93P/Lovas
05:00:43.42 +31:18:51.1 16.6mag 114P/Wiseman-Skiff
08:38:11.81 +29:13:01.0 15.1mag 123P/West-Hartley
11:10:57.95 -03:41:35.7 16.9mag 124P/Mrkos
05:10:58.10 +21:05:05.2 16.2mag 128P/Shoemaker-Holt
05:58:46.45 +19:31:17.9 17.8mag 131P/Mueller
07:55:36.52 +14:17:13.6 17.0mag 141P-D/Machholz
03:21:23.49 -20:28:51.1 14.9mag 161P/Hartley-IRAS
06:16:43.07 +36:09:33.1 15.5mag 162P/SidingSpring
18:19:47.86 +24:01:17.8 13.7mag 169P/NEAT
02:08:56.88 +08:45:00.1 17.6mag 220P/McNaught
16:35:56.40 -08:58:26.0 17.3mag 235P/LINEAR
20:35:01.04 -51:47:21.1 17.8mag 259P/Garradd
02:33:31.73 +17:43:28.4 15.5mag 260P/McNaught
06:14:10.00 +37:34:50.8 17.3mag 295P/LINEAR
15:06:52.49 +04:54:48.6 17.6mag 391P/Kowalski
08:45:33.30 +19:09:47.3 17.9mag 450P/LONEOS
08:10:33.90 +38:11:44.6 18.0mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.4K Jul 22 06:07 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
04:50:01.03 -02:22:33.80 ASASSN-26ej 2026-07-16.17 17.02
18:34:55.28 -31:41:00.90 ASASSN-26ek 2026-07-16.24 15.73
17:07:43.61 -44:21:53.50 ASASSN-26el 2026-07-15.86 16.01
14:45:08.35 +24:13:12.30 ASASSN-26ei 2026-07-16.17 16.46
10:00:46.44 -32:36:31.10 AT 2023mhb 2026-07-14.73 16.67
14:39:37.45 -11:22:36.20 AT 2026unl 2026-07-15.27 17.11
10:49:42.57 -11:25:55.80 ASASSN-26eh 2026-07-14.72 16.58
19:33:53.06 -07:15:00.80 ASASSN-26eg 2026-07-14.15 15.5
02:45:40.52 -27:55:30.30 ASASSN-26ef 2026-07-12.35 15.86
23:26:43.80 +04:42:39.70 SN 2026qtn 2026-07-12.22 16.47
02:19:17.26 +28:57:15.40 ASASSN-26ec 2026-07-11.53 2.78
18:31:15.56 -05:34:31.50 AT2026stb 2026-07-11.28 -1.29
13:36:08.24 +23:29:05.00 AT2026pjf 2026-07-10.18 -0.72
17:33:39.82 +04:22:36.70 SN2026pir 2026-07-9.86 -0.66
11:21:41.26 -50:33:36.30 ASASSN-26ed 2026-07-8.8 -1.3
23:41:42.11 +26:29:49.10 AT2026qil 2026-07-9.3 16.15
20:21:30.50 -32:03:40.10 ASASSN-26ee 2026-07-7.22 15.53
19:37:44.09 -05:35:42.80 AT2026ryu 2026-07-7.17 14.88
11:06:55.46 -04:07:04.50 AT2026qqg 2026-07-5.01 16.82
19:07:23.69 -74:13:37.30 AT2026qly 2026-07-5.02 17.31
17:57:43.80 +27:18:40.10 ASASSN-26ea 2026-07-5.07 16.67
19:59:01.43 -32:07:34.30 ASASSN-26eb 2026-07-4.97 15.52
18:46:50.35 -57:44:13.20 SN 2026qqp 2026-07-5.03 -0.92
19:17:31.69 -39:55:29.90 ASASSN-26dz 2026-07-5.14 15.91
19:14:31.37 +12:03:52.90 AT 2026rdg 2026-07-3.43 11.81
04:05:50.09 -70:24:34.40 AT 2026qpr 2026-06-30.4 15.96
13:45:37.49 -05:59:35.80 SN 2026pub 2026-06-30.09 16.01
16:41:15.63 +39:17:14.70 SN 2026pel 2026-06-26.38 16.07
10:14:40.19 -35:38:21.30 ASASSN-26dy 2026-06-25.99 15.63
14:47:21.56 -40:15:51.30 ASASSN-26dv 2026-06-23.03 14.62
13:38:49.79 -77:21:06.70 ASASSN-26dw 2026-06-23.04 16.09
00:59:27.90 +33:08:13.20 SN 2026mke 2026-06-22.39 17.13
11:10:44.73 -30:20:45.50 SN 2026nmv 2026-06-22.06 16.56
21:36:15.68 -21:19:12.50 AT2026oxh 2026-06-22.15 17.14
17:31:38.38 -56:05:51.90 ASASSN-26dx 2026-06-22.02 14.72
14:10:13.44 -38:46:46.10 AT2026pvk 2026-06-22.06 16.53
20:56:47.23 -18:31:05.20 AT2026plb 2026-06-21.31 16.4
15:44:29.68 +21:00:59.30 SN2026ore 2026-06-21.29 17.57
23:50:05.98 -14:01:41.30 AT2026oxl 2026-06-21.52 17.64
17:36:54.73 -18:10:04.20 AT2026ouj 2026-06-20.92 15.15
00:34:04.08 -30:22:09.20 AT2026ntk 2026-06-18.09 17.34
20:49:13.39 +25:17:59.20 ASASSN-26du 2026-06-15.39 15.93
23:09:30.84 +32:40:42.00 SN2026oxc 2026-06-14.35 16.83
02:02:26.78 +32:04:21.30 AT2026ovz 2026-06-14.59 15.39
21:26:28.11 -72:31:19.50 AT2026nwc 2026-06-11 17.05
17:54:57.33 +26:32:34.20 SN 2026odc 2026-06-11.23 17.62
13:55:59.94 +17:30:37.20 SN 2026nyq 2026-06-11.1 16.24
00:50:45.14 -71:38:36.90 ASASSN-26dt 2026-06-11.13 10.22
14:42:19.73 +19:11:35.60 SN2026nyp 2026-06-10.3 16.32
12:23:23.92 +12:56:43.50 SN2026mta 2026-06-8.29 16.69
12:30:18.51 +47:12:33.20 SN2026oao 2026-06-9.32 17.02
10:51:05.21 -42:28:56.60 AT2026nvf 2026-06-8.12 16.75
13:50:22.48 -07:35:00.00 SN2026npn 2026-06-8.02 17.58
00:56:07.17 +43:01:43.20 ASASSN-26dq 2026-06-7.43 13.58
01:07:49.46 +41:59:43.70 SN 2026obc 2026-06-7.43 15.15
21:11:25.22 +14:14:31.90 ASASSN-26dr 2026-06-7.24 16.24
06:21:27.06 -65:16:42.00 ASASSN-26ds 2026-06-2.97 15.02
20:07:38.15 -21:07:05.40 SN2026mho 2026-05-25.18 -1.12
11:29:42.55 +79:01:03.10 AT2026min 2026-05-24.21 16.63
11:44:32.95 -68:48:30.00 ASASSN-26no 2026-05-24 8.41
19:00:42.82 -48:31:01.60 ASASSN-26dp 2026-05-22.31 -3.28
14:23:56.72 -58:37:47.60 ASASSN-26dn 2026-05-20.01 14.64
11:24:54.06 +47:57:01.60 AT2026nma 2026-05-20.29 15.46
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
15:16:06.61 -79:16:32.40 ASASSN-26dm 2026-05-19.03 14.44
11:24:25.21 -59:23:19.10 ASASSN-26dl 2026-05-18.02 13.55
13:45:51.52 -53:16:01.00 ASASSN-26dk 2026-05-18.16 12.96
02:05:49.69 -30:29:09.60 ASASSN-26dh 2026-05-18.43 15.37
17:50:22.87 -39:42:33.90 ASASSN-26dj 2026-05-17.05 15.7
01:13:11.60 -33:25:16.10 ASASSN-26dg 2026-05-13.41 16.8
16:44:31.77 -27:15:18.40 AT2026mhn 2026-05-12.33 15.8
09:46:31.08 -33:41:51.00 ASASSN-26di 2026-05-12.14 14.63
21:23:11.57 -19:09:45.00 AT2026kwu 2026-05-12.26 16.9
14:20:14.30 -30:20:51.90 AT2026ktm 2026-05-12.06 17.21
14:41:39.01 -37:13:46.40 AT2026lkm 2026-05-11.18 16.89
12:59:50.45 -10:58:38.80 SN2026kep 2026-05-9.06 17.5
13:37:29.61 -29:50:30.90 AT2026lkd 2026-05-9.09 17.23
09:46:42.01 -14:52:03.60 SN2026kmo 2026-05-8.99 17.51
15:03:05.28 +22:02:03.80 AT2026lxf 2026-05-8.34 13.72
10:23:49.41 -20:57:25.30 ASASSN-26df 2026-05-8.21 16.52
22:14:40.56 +05:04:51.60 2026lda 2026-05-7.56 16.2
21:35:33.81 -14:05:16.30 ASASSN-26de 2026-05-6.29 14.51
16:21:49.13 -61:36:14.60 ASASSN-26dd 2026-05-5.15 15.93
14:26:40.22 -24:48:37.50 AT2026lig 2026-05-4.27 14.63
13:17:51.04 +30:25:13.50 SN2026kcp 2026-05-4.46 16.43
11:27:55.57 -13:38:56.90 SN2026kza 2026-05-1.08 15.59
22:28:27.10 +30:17:54.30 SN 2026fov 2026-04-29.6 14.36
21:00:10.71 -32:17:03.90 AT2026kis 2026-04-27.36 16.15
14:32:57.37 -58:13:26.40 ASASSN-26dc 2026-04-27.27 13.42
15:32:05.35 -43:54:34.60 ASASSN-26db 2026-04-27.37 16.06
16:34:34.97 -54:34:58.00 ASASSN-26da 2026-04-25.32 16.11
10:06:55.04 -01:13:49.70 SN2026jsg 2026-04-24.99 16.28
15:15:57.17 +56:18:32.80 SN2026kid 2026-04-24.52 -3.65
07:58:28.45 +57:03:42.40 AT2026kcf 2026-04-24.2 16.89
11:38:21.80 -50:43:06.50 SN2026jkb 2026-04-24.24 15.38
10:06:11.41 -39:41:04.20 AT2026dil 2026-04-24.2 16.85
14:21:40.08 +13:13:46.30 SN2026jlm 2026-04-22.16 15.12
10:53:55.52 -16:06:06.00 ASASSN-26cz 2026-04-22.28 16.29
04:50:01.03 -02:22:33.80 2026-07-16.17 17.02
-rw-r--r-- 1 apache apache 5.6K Jul 22 06:07 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
15:03:05.19 +22:02:04.1 TCP J15030519+2202041 2026-05-08.3260 13.9mag
07:15:18.25 +47:53:16.7 TCP J07151825+4753167 2026-05-09.1599 14.4mag
16:00:18.44 -22:30:10.6 TCP J16001844-2230106 2026-05-09.6135 13.3mag
00:42:47.45 +41:16:58.5 PNV J00424745+4116585 2026-05-10.030 16.8mag
09:55:02.89 +69:02:13.8 PNV J09550289+6902138 2026-05-18.925 20.7mag
00:43:01.82 +41:18:16.6 PNV J00430182+4118166 2026-05-21.8651 18.83Cmag
00:42:51.20 +41:16:59.4 PNV J00425120+4116594 2022-10-26.135 19.3mag
12:24:25.10 +28:47:12.0 TCP J12242510+2847120 2026-05-31.6015 14.8mag
00:56:07.13 +43:01:40.6 TCP J00560713+4301406 2026-06-01.4135 12.2mag
00:42:41.64 +41:15:16.2 PNV J00424164+4115162 2026-06-02.029 17.4mag
00:42:38.68 +41:15:58.2 PNV J00423868+4115582 2026-06-05.1224 19.97Umag
19:00:42.95 -48:31:01.7 PNV J19004295-4831017 2026-05-25.0752 14.2mag
09:55:21.28 +69:02:52.6 PNV J09552128+6902526 2026-06-13.933 18.9mag
19:51:21.42 +37:06:40.0 TCP J19512142+3706400 2026-06-17.2942 16.8mag
19:57:03.87 +37:41:46.4 TCP J19570387+3741464 2026-06-18.2638 17.5mag
00:42:32.04 +41:10:28.3 PNV J00423204+4110283 2026-06-26.059 16.6mag
02:19:17.36 +28:57:15.8 TCP J02191736+2857158 2026-07-12.3549 12.5mag
00:44:56.43 +41:57:41.6 PNV J00445643+4157416 2026-07-13.8026 17.98Cmag
00:42:55.36 +41:17:27.0 PNV J00425536+4117270 2026-07-20.1813 17.7mag
20:35:43.64 +61:31:32.9 TCP J20354364+6131329 2026-07-20.5443 14.4mag
-rw-r--r-- 1 apache apache 189K Jul 22 06:07 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
21:28:30.735 -13:12:02.42 AT 2026thq 2026-07-09.34 21.1053
23:15:36.302 -15:56:19.67 AT 2026thp 2026-07-09.35 22.954
20:46:17.542 -21:59:48.89 AT 2026tho 2026-07-09.29 22.7792
23:22:21.518 -04:57:52.50 AT 2026thn 2026-07-09.39 21.1667
04:01:26.281 -49:05:15.41 AT 2026thm 2026-07-09.42 23.5333
20:19:59.808 -11:52:00.26 AT 2026thl 2026-07-09.24 23.004
04:04:25.960 -49:17:10.25 AT 2026thk 2026-07-09.42 22.8309
20:18:30.116 -08:54:58.45 AT 2026thj 2026-07-09.27 23.008
19:31:06.780 -27:40:37.28 AT 2026thi 2026-07-09.31 22.3354
19:19:08.964 -20:49:20.86 AT 2026thh 2026-07-09.23 23.3724
23:09:35.488 -04:27:52.45 AT 2026thg 2026-07-09.35 22.3109
20:21:14.950 -12:37:31.63 AT 2026thf 2026-07-09.24 23.1886
20:14:38.286 -17:14:45.01 AT 2026the 2026-07-09.24 23.6002
19:29:06.461 -17:52:40.05 AT 2026thd 2026-07-09.23 22.8657
21:09:45.428 -13:55:34.32 AT 2026thc 2026-07-09.29 23.257
20:06:50.792 -15:37:22.53 AT 2026thb 2026-07-09.24 21.5403
23:09:49.547 -09:08:06.82 AT 2026tha 2026-07-09.35 22.9143
21:16:28.184 -15:45:09.49 AT 2026tgz 2026-07-09.29 23.0897
23:19:05.038 -08:43:55.11 AT 2026tgy 2026-07-09.35 21.7217
04:10:49.009 -48:43:16.73 AT 2026tgx 2026-07-09.42 22.2941
-rw-r--r-- 1 apache apache 88K Jul 22 06:07 tns_transients_list.txt
