This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Aur-01-Q1b1x1_022404_TTUQ1b1x1_62898_LWUeeVYZ
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 08 17.3077 2461269.8077 12.36 05:50:19.24 +56:29:05.9
156.31303 14.51735 galactic Cam Second-epoch detections are separated by 0.5" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:50:19.24 +56:29:05.9 (user input) | T | P | (position from user input) J-Ks=0.586+/-0.033 (K)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:50:19.24 +56:29:05.9: 13.29 +/- 0.03 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:50:19.24 +56:29:05.9: 13.36 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461269.8077,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260817.3077 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 17.3077 2461269.8077 12.52 05:29:54.09 +52:31:33.7
158.31651 9.97869 galactic Aur Second-epoch detections are separated by 2.2" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:29:54.09 +52:31:33.7 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.803+/-0.026 (K)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:29:54.09 +52:31:33.7: 13.42 +/- 0.03 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:29:54.09 +52:31:33.7: 13.44 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.43 +/- 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
target,2461269.8077,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260817.3077 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 17.3077 2461269.8077 12.60 05:53:22.42 +56:57:07.2
156.08111 15.10323 galactic Cam Second-epoch detections are separated by 2.2" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:53:22.42 +56:57:07.2 (user input) | T | P | (position from user input) J-Ks=0.669+/-0.033 (K)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:53:22.42 +56:57:07.2: 13.53 +/- 0.03 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:53:22.42 +56:57:07.2: 13.49 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.51 +/- 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
target,2461269.8077,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260817.3077 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 17.3077 2461269.8077 12.83 05:43:02.29 +56:26:26.1
155.86297 13.61012 galactic Cam Second-epoch detections are separated by 0.7" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:43:02.29 +56:26:26.1 (user input) | T | P | (position from user input) J-Ks=0.697+/-0.029 (K)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:43:02.29 +56:26:26.1: 13.78 +/- 0.04 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:43:02.29 +56:26:26.1: 13.85 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461269.8077,12.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260817.3077 12.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 17.3077 2461269.8077 12.75 04:54:24.73 +50:50:08.6
156.48487 4.52235 galactic Aur Second-epoch detections are separated by 1.1" and 6.5 pix
The object was found in VSX 2" ASASSN-V J045424.53+505008.0
Type: SR
# Max. Min./Amp. JD0 Period
15.650 g Y 0.370 g 2459105.04100 48.130000000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 04:54:24.73 +50:50:08.6: 13.89 +/- 0.06 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 04:54:24.73 +50:50:08.6: 13.91 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.90 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J045424.53+505008.0,2461269.8077,12.75,0.05,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 J045424.53+505008.0 20260817.3077 12.75CV 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 08 17.3077 2461269.8077 12.83 05:44:15.90 +55:09:50.1
157.09707 13.14310 galactic Aur Second-epoch detections are separated by 0.5" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:44:15.90 +55:09:50.1 (user input) | T | P | (position from user input) J-Ks=0.435+/-0.029 (G)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:44:15.90 +55:09:50.1: 13.88 +/- 0.04 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:44:15.90 +55:09:50.1: 13.71 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.77 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461269.8077,12.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260817.3077 12.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 17.3077 2461269.8077 12.82 05:34:52.94 +51:53:03.7
159.27841 10.29083 galactic Aur Second-epoch detections are separated by 4.3" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:34:52.94 +51:53:03.7 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.386+/-0.030 (G)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:34:52.94 +51:53:03.7: 13.85 +/- 0.04 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:34:52.94 +51:53:03.7: 13.85 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.85 +/- 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
target,2461269.8077,12.82,0.05,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
target 20260817.3077 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 08 17.3077 2461269.8077 12.84 06:01:21.71 +57:12:11.1
156.34128 16.18872 galactic Cam Second-epoch detections are separated by 2.9" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:01:21.71 +57:12:11.1 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.643+/-0.030 (K)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 06:01:21.71 +57:12:11.1: 13.85 +/- 0.05 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 06:01:21.71 +57:12:11.1: 13.95 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.90 +/- 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
target,2461269.8077,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260817.3077 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 17.3077 2461269.8077 12.82 05:47:18.83 +55:50:29.5
156.69777 13.84648 galactic Aur Second-epoch detections are separated by 1.5" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:47:18.83 +55:50:29.5 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.333+/-0.030 (G)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:47:18.83 +55:50:29.5: 13.87 +/- 0.05 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:47:18.83 +55:50:29.5: 13.84 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.85 +/- 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
target,2461269.8077,12.82,0.05,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
target 20260817.3077 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 08 17.3077 2461269.8077 12.81 05:34:58.07 +53:25:58.2
157.93671 11.10313 galactic Aur Second-epoch detections are separated by 1.0" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:34:58.07 +53:25:58.2 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.354+/-0.030 (G)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:34:58.07 +53:25:58.2: 13.83 +/- 0.05 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:34:58.07 +53:25:58.2: 13.77 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.80 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461269.8077,12.81,0.05,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
target 20260817.3077 12.81CV 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 08 17.3077 2461269.8077 12.81 05:40:38.78 +53:24:10.7
158.40111 11.81695 galactic Aur Second-epoch detections are separated by 4.3" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:40:38.78 +53:24:10.7 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.760+/-0.027 (K)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:40:38.78 +53:24:10.7: 13.82 +/- 0.04 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:40:38.78 +53:24:10.7: 13.82 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.82 +/- 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
target,2461269.8077,12.81,0.05,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
target 20260817.3077 12.81CV 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 08 17.3077 2461269.8077 12.78 04:57:45.79 +51:36:13.2
156.20954 5.41106 galactic Aur Second-epoch detections are separated by 2.0" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.4460+51.6023 | 04:57:45.79 +51:36:13.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.658+/-0.044 (Very red! L if it's a dwarf)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 04:57:45.79 +51:36:13.2: 13.83 +/- 0.05 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 04:57:45.79 +51:36:13.2: 13.79 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J074.4460+51.6023,2461269.8077,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J074.4460+51.6023 20260817.3077 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 17.3077 2461269.8077 12.84 05:54:47.45 +57:19:44.9
155.82102 15.44416 galactic Cam Second-epoch detections are separated by 2.2" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:54:47.45 +57:19:44.9 (user input) | T | P | (position from user input) J-Ks=0.840+/-0.029 (M)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:54:47.45 +57:19:44.9: 13.82 +/- 0.05 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:54:47.45 +57:19:44.9: 13.92 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.87 +/- 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
target,2461269.8077,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260817.3077 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 17.3077 2461269.8077 12.76 05:32:47.75 +50:53:24.3
159.96554 9.49312 galactic Aur Second-epoch detections are separated by 1.9" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:32:47.75 +50:53:24.3 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.751+/-0.029 (K)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:32:47.75 +50:53:24.3: 13.80 +/- 0.04 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:32:47.75 +50:53:24.3: 13.79 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.80 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461269.8077,12.76,0.05,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
target 20260817.3077 12.76CV 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 08 17.3077 2461269.8077 12.81 05:50:02.10 +56:08:33.1
156.60748 14.32366 galactic Cam Second-epoch detections are separated by 2.8" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:50:02.10 +56:08:33.1 (user input) | T | P | (position from user input) J-Ks=0.528+/-0.035 (K)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:50:02.10 +56:08:33.1: 13.80 +/- 0.04 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:50:02.10 +56:08:33.1: 13.82 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461269.8077,12.81,0.05,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
target 20260817.3077 12.81CV 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 08 17.3077 2461269.8077 12.82 05:40:14.81 +54:02:48.2
157.80083 12.08720 galactic Aur Second-epoch detections are separated by 1.6" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:40:14.81 +54:02:48.2 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.796+/-0.030 (K)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:40:14.81 +54:02:48.2: 13.78 +/- 0.04 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:40:14.81 +54:02:48.2: 13.71 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.74 +/- 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
target,2461269.8077,12.82,0.05,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
target 20260817.3077 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 08 17.3077 2461269.8077 12.81 05:39:37.99 +54:33:15.3
157.30522 12.26295 galactic Aur Second-epoch detections are separated by 1.4" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:39:37.99 +54:33:15.3 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.706+/-0.030 (K)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:39:37.99 +54:33:15.3: 13.76 +/- 0.03 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:39:37.99 +54:33:15.3: 13.81 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.78 +/- 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
target,2461269.8077,12.81,0.05,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
target 20260817.3077 12.81CV 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 08 17.3077 2461269.8077 12.76 05:37:53.88 +53:58:59.9
157.67972 11.75701 galactic Aur Second-epoch detections are separated by 0.6" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:37:53.88 +53:58:59.9 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.727+/-0.030 (K)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:37:53.88 +53:58:59.9: 13.77 +/- 0.04 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:37:53.88 +53:58:59.9: 13.75 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.76 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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
target,2461269.8077,12.76,0.05,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
target 20260817.3077 12.76CV 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 08 17.3077 2461269.8077 12.85 05:31:42.82 +52:59:28.1
158.06253 10.45725 galactic Aur Second-epoch detections are separated by 1.2" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:31:42.82 +52:59:28.1 (user input) | T | P | (position from user input) J-Ks=0.827+/-0.029 (M)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:31:42.82 +52:59:28.1: 13.74 +/- 0.04 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:31:42.82 +52:59:28.1: 13.76 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.75 +/- 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
target,2461269.8077,12.85,0.05,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
target 20260817.3077 12.85CV 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 08 17.3077 2461269.8077 12.81 05:26:53.09 +51:50:32.7
158.65018 9.22181 galactic Aur Second-epoch detections are separated by 1.6" and 6.6 pix
The object was found in VSX 1" ASASSN-V J052653.14+515032.3
Type: SR
# Max. Min./Amp. JD0 Period
14.100 V 14.370 V 2457403.80000 75.700000000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:26:53.09 +51:50:32.7: 13.78 +/- 0.04 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:26:53.09 +51:50:32.7: 13.72 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.75 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J052653.14+515032.3,2461269.8077,12.81,0.05,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
ASASSN-V J052653.14+515032.3 20260817.3077 12.81CV 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 08 17.3077 2461269.8077 12.79 05:38:46.03 +52:40:16.0
158.90144 11.20454 galactic Aur Second-epoch detections are separated by 3.6" and 6.1 pix
The object was found in VSX19" Gaia DR3 263689688938335360
Type: S
# Max. Min./Amp. JD0 Period
16.710 G 17.080 G
ATTENTION: measured mag 12.79 is 3.9 mag brighter than the VSX record maximum brightness 16.71 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:38:46.03 +52:40:16.0: 13.72 +/- 0.03 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:38:46.03 +52:40:16.0: 13.71 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.71 +/- 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
Gaia DR3 263689688938335360,2461269.8077,12.79,0.05,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
Gaia DR3 263689688938335360 20260817.3077 12.79CV 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 08 17.3077 2461269.8077 12.87 05:41:29.43 +54:38:58.8
157.35715 12.54380 galactic Aur Second-epoch detections are separated by 1.5" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J085.3849+54.6527 | 05:41:29.43 +54:38:58.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F2 (LAMOST DR5)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:41:29.43 +54:38:58.8: 13.76 +/- 0.04 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:41:29.43 +54:38:58.8: 13.77 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.77 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J085.3849+54.6527,2461269.8077,12.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J085.3849+54.6527 20260817.3077 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 17.3077 2461269.8077 12.71 05:40:15.14 +54:17:29.3
157.58423 12.20994 galactic Aur Second-epoch detections are separated by 3.9" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:40:15.14 +54:17:29.3 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.706+/-0.025 (K)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:40:15.14 +54:17:29.3: 13.72 +/- 0.04 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:40:15.14 +54:17:29.3: 13.65 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.68 +/- 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
target,2461269.8077,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260817.3077 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 17.3077 2461269.8077 12.78 05:50:07.59 +56:13:10.7
156.54306 14.37070 galactic Cam Second-epoch detections are separated by 0.9" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:50:07.59 +56:13:10.7 (user input) | T | P | (position from user input) J-Ks=0.308+/-0.037 (F)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:50:07.59 +56:13:10.7: 13.71 +/- 0.04 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:50:07.59 +56:13:10.7: 13.72 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.72 +/- 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
target,2461269.8077,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260817.3077 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 17.3077 2461269.8077 12.80 05:32:04.11 +50:32:36.9
160.20198 9.21225 galactic Aur Second-epoch detections are separated by 3.7" and 6.9 pix
The object was found in VSX 1" ZTF J053204.06+503237.4
Type: SR
# Max. Min./Amp. JD0 Period
14.589 g Y 0.287 g 2458513.55210 30.864164800000
The object was not found in astcheck.
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:32:04.11 +50:32:36.9: 13.74 +/- 0.04 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:32:04.11 +50:32:36.9: 13.74 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.74 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J053204.06+503237.4,2461269.8077,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J053204.06+503237.4 20260817.3077 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 17.3077 2461269.8077 12.79 05:43:20.94 +53:14:52.8
158.74328 12.09047 galactic Aur Second-epoch detections are separated by 2.6" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J085.8296+53.2456 | 05:43:20.94 +53:14:52.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G6 (LAMOST DR5) J-Ks=0.492+/-0.029 (K)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:43:20.94 +53:14:52.8: 13.71 +/- 0.04 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:43:20.94 +53:14:52.8: 13.70 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.70 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J085.8296+53.2456,2461269.8077,12.79,0.05,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
ATO J085.8296+53.2456 20260817.3077 12.79CV 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 08 17.3077 2461269.8077 12.74 04:57:46.41 +50:25:34.1
157.13946 4.68406 galactic Aur Second-epoch detections are separated by 1.1" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:57:46.41 +50:25:34.1 (user input) | T | P | (position from user input) J-Ks=0.877+/-0.033 (M)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 04:57:46.41 +50:25:34.1: 13.70 +/- 0.05 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 04:57:46.41 +50:25:34.1: 13.67 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.68 +/- 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
target,2461269.8077,12.74,0.05,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
target 20260817.3077 12.74CV 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 08 17.3077 2461269.8077 12.66 05:53:27.12 +57:10:27.0
155.88062 15.21287 galactic Cam Second-epoch detections are separated by 2.5" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:53:27.12 +57:10:27.0 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.711+/-0.030 (K)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:53:27.12 +57:10:27.0: 13.72 +/- 0.04 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:53:27.12 +57:10:27.0: 13.64 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461269.8077,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260817.3077 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 17.3077 2461269.8077 12.70 05:35:32.95 +53:53:37.0
157.57884 11.41385 galactic Aur Second-epoch detections are separated by 1.7" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:35:32.95 +53:53:37.0 (user input) | T | P | (position from user input) J-Ks=0.558+/-0.029 (K)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:35:32.95 +53:53:37.0: 13.68 +/- 0.03 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:35:32.95 +53:53:37.0: 13.71 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.70 +/- 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
target,2461269.8077,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260817.3077 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 17.3077 2461269.8077 12.78 05:44:05.84 +55:40:28.7
156.62599 13.36928 galactic Aur Second-epoch detections are separated by 1.8" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:44:05.84 +55:40:28.7 (user input) | T | P | (position from user input) SpType: K7 (LAMOST DR5) J-Ks=0.779+/-0.030 (K)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:44:05.84 +55:40:28.7: 13.69 +/- 0.04 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:44:05.84 +55:40:28.7: 13.70 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.69 +/- 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
target,2461269.8077,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260817.3077 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 17.3077 2461269.8077 12.76 05:20:36.38 +49:48:13.2
159.81657 7.27071 galactic Aur Second-epoch detections are separated by 3.5" and 7.0 pix
The object was found in VSX 1" ASASSN-V J052036.52+494813.0
Type: SRS
# Max. Min./Amp. JD0 Period
13.920 V 14.020 V 2458066.06700 19.859000000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:20:36.38 +49:48:13.2: 13.70 +/- 0.04 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:20:36.38 +49:48:13.2: 13.73 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.71 +/- 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 J052036.52+494813.0,2461269.8077,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J052036.52+494813.0 20260817.3077 12.76CV 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 08 17.3077 2461269.8077 12.72 05:07:34.64 +49:24:22.7
158.91457 5.31901 galactic Aur Second-epoch detections are separated by 4.3" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:07:34.64 +49:24:22.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:07:34.64 +49:24:22.7: 13.66 +/- 0.04 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:07:34.64 +49:24:22.7: 13.59 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.62 +/- 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
target,2461269.8077,12.72,0.05,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
target 20260817.3077 12.72CV 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 08 17.3077 2461269.8077 12.71 05:46:04.02 +55:39:55.4
156.77148 13.60843 galactic Aur Second-epoch detections are separated by 2.5" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:46:04.02 +55:39:55.4 (user input) | T | P | (position from user input) J-Ks=0.572+/-0.029 (K)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:46:04.02 +55:39:55.4: 13.63 +/- 0.04 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:46:04.02 +55:39:55.4: 13.63 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.63 +/- 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
target,2461269.8077,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260817.3077 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 17.3077 2461269.8077 12.69 05:42:54.04 +54:52:53.3
157.25265 12.83484 galactic Aur Second-epoch detections are separated by 0.1" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J085.7310+54.8808 | 05:42:54.04 +54:52:53.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.606+/-0.028 (K)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:42:54.04 +54:52:53.3: 13.63 +/- 0.03 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:42:54.04 +54:52:53.3: 13.56 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.59 +/- 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
ATO J085.7310+54.8808,2461269.8077,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J085.7310+54.8808 20260817.3077 12.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 17.3077 2461269.8077 12.71 05:52:07.90 +56:52:53.8
156.06654 14.92025 galactic Cam Second-epoch detections are separated by 2.4" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:52:07.90 +56:52:53.8 (user input) | T | P | (position from user input) J-Ks=0.831+/-0.034 (M)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:52:07.90 +56:52:53.8: 13.64 +/- 0.04 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:52:07.90 +56:52:53.8: 13.59 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.61 +/- 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
target,2461269.8077,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260817.3077 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 17.3077 2461269.8077 12.59 05:38:55.51 +55:58:52.7
155.98601 12.88653 galactic Aur Second-epoch detections are separated by 1.1" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:38:55.51 +55:58:52.7 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.749+/-0.024 (K)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:38:55.51 +55:58:52.7: 13.62 +/- 0.03 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:38:55.51 +55:58:52.7: 13.57 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.60 +/- 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
target,2461269.8077,12.59,0.05,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
target 20260817.3077 12.59CV 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 08 17.3077 2461269.8077 12.69 05:35:22.99 +53:16:01.5
158.11402 11.07089 galactic Aur Second-epoch detections are separated by 1.2" and 6.5 pix
The object was found in VSX 2" HAT-094-0007885
Type: BY+UV
# Max. Min./Amp. JD0 Period
13.800 V Y 0.219 V 4.307857000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:35:22.99 +53:16:01.5: 13.60 +/- 0.03 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:35:22.99 +53:16:01.5: 13.61 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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
HAT-094-0007885,2461269.8077,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT-094-0007885 20260817.3077 12.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 17.3077 2461269.8077 12.63 05:35:41.59 +53:53:29.7
157.59171 11.43103 galactic Aur Second-epoch detections are separated by 1.1" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:35:41.59 +53:53:29.7 (user input) | T | P | (position from user input) J-Ks=0.897+/-0.028 (M)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:35:41.59 +53:53:29.7: 13.58 +/- 0.03 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:35:41.59 +53:53:29.7: 13.69 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.63 +/- 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
target,2461269.8077,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260817.3077 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 17.3077 2461269.8077 12.68 05:41:05.59 +54:34:29.4
157.39465 12.45680 galactic Aur Second-epoch detections are separated by 0.6" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:41:05.59 +54:34:29.4 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.734+/-0.032 (K)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:41:05.59 +54:34:29.4: 13.58 +/- 0.03 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:41:05.59 +54:34:29.4: 13.63 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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
target,2461269.8077,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260817.3077 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 17.3077 2461269.8077 12.65 05:43:16.88 +55:14:46.9
156.95311 13.06044 galactic Aur Second-epoch detections are separated by 1.0" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:43:16.88 +55:14:46.9 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.829+/-0.029 (M)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:43:16.88 +55:14:46.9: 13.57 +/- 0.03 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:43:16.88 +55:14:46.9: 13.57 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.57 +/- 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
target,2461269.8077,12.65,0.05,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
target 20260817.3077 12.65CV 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 08 17.3077 2461269.8077 12.54 05:46:54.01 +55:50:01.2
156.67657 13.79161 galactic Aur Second-epoch detections are separated by 0.7" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J086.7178+55.8345 | 05:46:54.01 +55:50:01.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.842+/-0.027 (M)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:46:54.01 +55:50:01.2: 13.54 +/- 0.03 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:46:54.01 +55:50:01.2: 13.53 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.54 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J086.7178+55.8345,2461269.8077,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J086.7178+55.8345 20260817.3077 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 17.3077 2461269.8077 12.62 06:02:54.74 +57:40:37.8
155.98535 16.57816 galactic Cam Second-epoch detections are separated by 2.2" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:02:54.74 +57:40:37.8 (user input) | T | P | (position from user input) J-Ks=0.339+/-0.035 (G)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 06:02:54.74 +57:40:37.8: 13.52 +/- 0.04 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 06:02:54.74 +57:40:37.8: 13.53 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.52 +/- 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
target,2461269.8077,12.62,0.05,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
target 20260817.3077 12.62CV 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 08 17.3077 2461269.8077 12.55 05:55:06.04 +57:07:01.8
156.03726 15.38728 galactic Cam Second-epoch detections are separated by 1.6" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:55:06.04 +57:07:01.8 (user input) | T | P | (position from user input) J-Ks=0.351+/-0.033 (G)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:55:06.04 +57:07:01.8: 13.48 +/- 0.03 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:55:06.04 +57:07:01.8: 13.50 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.49 +/- 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
target,2461269.8077,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260817.3077 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 17.3077 2461269.8077 12.53 05:42:46.09 +54:44:39.6
157.36571 12.75108 galactic Aur Second-epoch detections are separated by 0.1" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J085.6891+54.7463 | 05:42:46.09 +54:44:39.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.107+/-0.028 (M)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:42:46.09 +54:44:39.6: 13.48 +/- 0.03 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:42:46.09 +54:44:39.6: 13.44 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J085.6891+54.7463,2461269.8077,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J085.6891+54.7463 20260817.3077 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 17.3077 2461269.8077 12.54 06:03:34.05 +57:50:33.0
155.86669 16.72664 galactic Cam Second-epoch detections are separated by 1.9" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:03:34.05 +57:50:33.0 (user input) | T | P | (position from user input) J-Ks=0.336+/-0.069 (G)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 06:03:34.05 +57:50:33.0: 13.48 +/- 0.03 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 06:03:34.05 +57:50:33.0: 13.43 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461269.8077,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260817.3077 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 17.3077 2461269.8077 12.48 05:35:01.42 +54:18:43.4
157.17195 11.56230 galactic Aur Second-epoch detections are separated by 1.5" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:35:01.42 +54:18:43.4 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.435+/-0.027 (G)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:35:01.42 +54:18:43.4: 13.46 +/- 0.03 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:35:01.42 +54:18:43.4: 13.47 +/- 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
target,2461269.8077,12.48,0.05,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
target 20260817.3077 12.48CV 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 08 17.3077 2461269.8077 12.54 05:57:39.19 +57:38:03.1
155.71262 15.92389 galactic Cam Second-epoch detections are separated by 0.7" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:57:39.19 +57:38:03.1 (user input) | T | P | (position from user input) J-Ks=0.688+/-0.027 (K)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:57:39.19 +57:38:03.1: 13.44 +/- 0.03 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:57:39.19 +57:38:03.1: 13.55 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.49 +/- 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
target,2461269.8077,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260817.3077 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 17.3077 2461269.8077 12.49 06:04:24.29 +58:22:52.0
155.40218 17.05032 galactic Cam Second-epoch detections are separated by 1.4" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:04:24.29 +58:22:52.0 (user input) | T | P | (position from user input) J-Ks=0.402+/-0.043 (G)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 06:04:24.29 +58:22:52.0: 13.43 +/- 0.03 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 06:04:24.29 +58:22:52.0: 13.44 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.43 +/- 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
target,2461269.8077,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260817.3077 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 17.3077 2461269.8077 12.44 05:40:22.07 +55:45:24.0
156.28907 12.95103 galactic Aur Second-epoch detections are separated by 1.4" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:40:22.07 +55:45:24.0 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.664+/-0.030 (K)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:40:22.07 +55:45:24.0: 13.40 +/- 0.03 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:40:22.07 +55:45:24.0: 13.39 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin 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
target,2461269.8077,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260817.3077 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 17.3077 2461269.8077 12.48 05:42:40.50 +56:20:38.0
155.92494 13.51932 galactic Cam Second-epoch detections are separated by 1.3" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J085.6791+56.3341 | 05:42:40.50 +56:20:38.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.410+/-0.030 (G)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:42:40.50 +56:20:38.0: 13.39 +/- 0.03 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:42:40.50 +56:20:38.0: 13.46 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.42 +/- 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
ATO J085.6791+56.3341,2461269.8077,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J085.6791+56.3341 20260817.3077 12.48CV 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 08 17.3077 2461269.8077 12.48 05:57:54.51 +57:21:52.1
155.98056 15.83722 galactic Cam Second-epoch detections are separated by 1.6" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:57:54.51 +57:21:52.1 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.361+/-0.032 (G)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:57:54.51 +57:21:52.1: 13.39 +/- 0.03 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:57:54.51 +57:21:52.1: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.39 +/- 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
target,2461269.8077,12.48,0.05,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
target 20260817.3077 12.48CV 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 08 17.3077 2461269.8077 12.51 05:26:01.58 +51:33:53.2
158.81331 8.95945 galactic Aur Second-epoch detections are separated by 0.9" and 6.4 pix
The object was not found in VSX
The object was found in ASASSN-V 0" ASASSN-V J052601.62+513353.6
Type: SR
MeanMag 13.71 m Amp. 0.1 m Period 21.9546809 d
The object was not found in astcheck.
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:26:01.58 +51:33:53.2: 13.40 +/- 0.03 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:26:01.58 +51:33:53.2: 13.49 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.44 +/- 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
VARIABLE_NAME,2461269.8077,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260817.3077 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 17.3077 2461269.8077 12.36 05:34:17.21 +51:20:54.3
159.69425 9.93279 galactic Aur Second-epoch detections are separated by 0.7" and 6.4 pix
The object was found in VSX 1" ASASSN-V J053417.20+512053.8
Type: SRS
# Max. Min./Amp. JD0 Period
13.440 V 13.530 V 2457984.11600 25.961000000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:34:17.21 +51:20:54.3: 13.28 +/- 0.02 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:34:17.21 +51:20:54.3: 13.32 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J053417.20+512053.8,2461269.8077,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J053417.20+512053.8 20260817.3077 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 17.3077 2461269.8077 12.38 06:02:41.20 +58:29:42.4
155.19637 16.89286 galactic Cam Second-epoch detections are separated by 0.7" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:02:41.20 +58:29:42.4 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.333+/-0.032 (G)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 06:02:41.20 +58:29:42.4: 13.25 +/- 0.03 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 06:02:41.20 +58:29:42.4: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.27 +/- 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
target,2461269.8077,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260817.3077 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 17.3077 2461269.8077 12.12 05:38:32.79 +53:39:11.5
158.02003 11.67279 galactic Aur Second-epoch detections are separated by 0.4" and 6.3 pix
The object was found in VSX 1" ASASSN-V J053832.78+533912.3
Type: SR
# Max. Min./Amp. JD0 Period
13.340 V 13.530 V 2457419.80000 41.410000000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:38:32.79 +53:39:11.5: 13.11 +/- 0.02 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:38:32.79 +53:39:11.5: 13.16 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J053832.78+533912.3,2461269.8077,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J053832.78+533912.3 20260817.3077 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 17.3077 2461269.8077 12.13 05:42:37.11 +55:26:33.0
156.73015 13.07377 galactic Aur Second-epoch detections are separated by 1.3" and 6.0 pix
The object was found in VSX 0" Gaia DR3 265127781426681472
Type: RS
# Max. Min./Amp. JD0 Period
12.490 G 12.710 G K
The object was not found in astcheck.
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:42:37.11 +55:26:33.0: 13.06 +/- 0.02 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:42:37.11 +55:26:33.0: 13.11 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.08 +/- 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
Gaia DR3 265127781426681472,2461269.8077,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 265127781426681472 20260817.3077 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 17.3077 2461269.8077 11.79 06:04:44.89 +57:46:52.6
155.99301 16.84431 galactic Cam Second-epoch detections are separated by 0.3" and 5.8 pix
The object was found in VSX 1" NEV289
Type: EA
# Max. Min./Amp. JD0 Period
12.400 V 13.200 V 2458538.35200 6.793630000000 G7
The object was not found in astcheck.
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 06:04:44.89 +57:46:52.6: 12.68 +/- 0.02 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 06:04:44.89 +57:46:52.6: 12.68 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.68 +/- 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
NEV289,2461269.8077,11.79,0.05,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
NEV289 20260817.3077 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 08 17.3077 2461269.8077 13.04 05:37:39.51 +54:06:44.7
157.54779 11.79201 galactic Aur Second-epoch detections are separated by 4.3" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:37:39.51 +54:06:44.7 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.901+/-0.029 (M)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:37:39.51 +54:06:44.7: 14.29 +/- 0.06 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:37:39.51 +54:06:44.7: 14.23 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.26 +/- 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
target,2461269.8077,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260817.3077 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 17.3077 2461269.8077 12.99 05:34:37.49 +53:38:03.0
157.73412 11.16328 galactic Aur Second-epoch detections are separated by 2.8" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J083.6699+53.6388 | 05:34:37.49 +53:38:03.0 (user input) | IRR (ATLAS) | (ATLAS) | (position from user input) SpType: F9 (LAMOST DR5)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:34:37.49 +53:38:03.0: 14.10 +/- 0.05 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:34:37.49 +53:38:03.0: 14.03 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.06 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J083.6699+53.6388,2461269.8077,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J083.6699+53.6388 20260817.3077 12.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 17.3077 2461269.8077 12.89 05:37:03.11 +53:58:27.8
157.62315 11.64526 galactic Aur Second-epoch detections are separated by 0.5" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:37:03.11 +53:58:27.8 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.815+/-0.026 (M)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:37:03.11 +53:58:27.8: 14.06 +/- 0.05 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:37:03.11 +53:58:27.8: 14.07 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.06 +/- 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
target,2461269.8077,12.89,0.05,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
target 20260817.3077 12.89CV 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 08 17.3077 2461269.8077 13.02 05:34:17.98 +52:16:29.8
158.89190 10.41734 galactic Aur Second-epoch detections are separated by 1.2" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:34:17.98 +52:16:29.8 (user input) | T | P | (position from user input) SpType: K5 (LAMOST DR5) J-Ks=0.713+/-0.027 (K)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:34:17.98 +52:16:29.8: 14.05 +/- 0.05 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:34:17.98 +52:16:29.8: 14.13 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.08 +/- 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
target,2461269.8077,13.02,0.05,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
target 20260817.3077 13.02CV 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 08 17.3077 2461269.8077 12.96 05:40:04.30 +54:14:54.8
157.60884 12.16567 galactic Aur Second-epoch detections are separated by 1.3" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:40:04.30 +54:14:54.8 (user input) | T | P | (position from user input) SpType: G6 (LAMOST DR5) J-Ks=0.532+/-0.026 (K)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:40:04.30 +54:14:54.8: 14.01 +/- 0.05 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:40:04.30 +54:14:54.8: 14.12 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.06 +/- 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
target,2461269.8077,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260817.3077 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 17.3077 2461269.8077 12.84 05:48:48.39 +56:10:18.3
156.49858 14.18593 galactic Cam Second-epoch detections are separated by 1.7" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:48:48.39 +56:10:18.3 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.388+/-0.037 (G)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:48:48.39 +56:10:18.3: 14.01 +/- 0.05 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:48:48.39 +56:10:18.3: 14.02 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.02 +/- 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
target,2461269.8077,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260817.3077 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 17.3077 2461269.8077 12.95 05:31:50.03 +50:50:01.1
159.93278 9.33442 galactic Aur Second-epoch detections are separated by 4.0" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J082.9585+50.8338 | 05:31:50.03 +50:50:01.1 (user input) | IRR (ATLAS) | (ATLAS) | (position from user input) SpType: M0 (LAMOST DR5) J-Ks=1.230+/-0.025 (M)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:31:50.03 +50:50:01.1: 13.97 +/- 0.05 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:31:50.03 +50:50:01.1: 13.92 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.94 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J082.9585+50.8338,2461269.8077,12.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J082.9585+50.8338 20260817.3077 12.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461058.74181476 18.01.2026 05:48:02.795 /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits
First image: 2461058.74181476 18.01.2026 05:48:02.795 /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits
Last image: 2461269.80806524 17.08.2026 07:23:26.837 /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Aur-01-Q1b1x1_022404_TTUQ1b1x1_62898_LWUeeVYZ/fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.56
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 5 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 18549
Objects passed selection criteria: 18420
Measurements per detected object (mean, median, min, max): 2.3 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.3 2.0 2 4
Average stars detected per image: 11461.8
Average stars matched: 11164 (97.4022 %)
Memory usage VmPeak: 243660 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Aug 14 19:27:11 CDT 2026
VaST build number 1.0rc89-191-g1c132b07
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-14)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Aug 17 02:28:38 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461058.74181476 18.01.2026 05:48:02.795 /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits
First image: 2461058.74181476 18.01.2026 05:48:02.795 /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits
Last image: 2461269.80806524 17.08.2026 07:23:26.837 /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Aur-01-Q1b1x1_022404_TTUQ1b1x1_62898_LWUeeVYZ/fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 126
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.26
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: 27 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 128816
Objects passed selection criteria: 128412
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: 84900.2
Average stars matched: 81510.8 (96.0077 %)
Memory usage VmPeak: 596832 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Aug 14 19:27:11 CDT 2026
VaST build number 1.0rc89-191-g1c132b07
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-14)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Aug 17 02:29:41 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-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Aur-01-Q1b1x1_022404_TTUQ1b1x1_62898_LWUeeVYZ/fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Aur-01-Q1b1x1_022404_TTUQ1b1x1_62898_LWUeeVYZ/fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits
SExtractor catalog cache: saved Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits.cat to cache
SExtractor catalog cache: saved Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.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-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Aur-01-Q1b1x1_022404_TTUQ1b1x1_62898_LWUeeVYZ/fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Aur-01-Q1b1x1_022404_TTUQ1b1x1_62898_LWUeeVYZ/fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.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: 2461269.80728188
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-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits exists and is non-empty
wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits exists and is non-empty
wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits exists and is non-empty
wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits (1st reference image)
verification OK: wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits
Image size: 941.7'x627.2' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:38:52.744 +53:59:24.28 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-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits (1st new image)
verification OK: wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits
Image size: 944.3'x627.0' 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: 05:38:47.497 +53:58:50.52 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:38:52.744 +53:59:24.28
Second-epoch image center 05:38:47.497 +53:58:50.52
Angular distance between the image centers 0.0159 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits (2nd new image)
verification OK: wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits
Image size: 944.2'x627.0' 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: 05:38:45.550 +53:59:23.35 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:38:52.744 +53:59:24.28
Second-epoch image center 05:38:45.550 +53:59:23.35
Angular distance between the image centers 0.0176 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 05:38:47.497 +53:58:50.52
Second-epoch second image center 05:38:45.550 +53:59:23.35
Angular distance between the image centers 0.01029 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-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits &> /tmp/tmp.sSPkvLZ8yM
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits &> /tmp/tmp.e4VCAyJVDG
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Aur-01-Q1b1x1_022404_TTUQ1b1x1_62898_LWUeeVYZ/fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits &> /tmp/tmp.yz0P5KQHry
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Aur-01-Q1b1x1_022404_TTUQ1b1x1_62898_LWUeeVYZ/fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Aur-01-Q1b1x1_022404_TTUQ1b1x1_62898_LWUeeVYZ/fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits &> /tmp/tmp.GuDPDDQOcI
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Aur-01-Q1b1x1_022404_TTUQ1b1x1_62898_LWUeeVYZ/fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.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-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits and wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.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-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits and wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits.wcscat
Found non-empty wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits and wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits.wcscat
The reference image (wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits) and catalog (wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits.wcscat) found
'wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits.wcscat' -> 'wcsmag.cat'
Read 19819 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 70.2032 to 100.1189 deg, Dec +47.7367 to +59.3617 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 70.2032 to 100.1189 deg, Dec 47.7367 to 59.3617 deg
Loaded 11634 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): 7484 out of 8218 total matches.
Matched with Tycho-2 8218 out of 19819 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.910150
a=0.000000 b=1.000000 c=22.910150
From vast_summary.log: estimated ref. image limiting mag.: -7.56
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.35
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.35
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 19819 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 70.2032 to 100.1189 deg, Dec +47.7367 to +59.3617 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 70.2032 to 100.1189 deg, Dec 47.7367 to 59.3617 deg
Loaded 11634 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): 7484 out of 8218 total matches.
Matched with Tycho-2 8218 out of 19819 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits
Forced-photometry filter: calibrated wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits -> calib.txt_param_ref_wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits (aperture=6.2)
Read 19771 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 70.2032 to 100.1191 deg, Dec +47.7368 to +59.3412 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 70.2032 to 100.1191 deg, Dec 47.7368 to 59.3412 deg
Loaded 11612 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): 7500 out of 8210 total matches.
Matched with Tycho-2 8210 out of 19771 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits
Forced-photometry filter: calibrated wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits -> calib.txt_param_ref_wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits (aperture=6.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits
2.1 pix Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits
2.5 pix fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits
2.5 pix fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits
Limiting magnitude estimates:
15.3 mag. Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits
15.3 mag. Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits
12.5 mag. fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits
12.6 mag. fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits
All-image limiting magnitude estimate: 12.5 (SNR ) 10.6 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.sSPkvLZ8yM (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_2026-08-17_CI_Aur-01-Q1b1x1_022404_TTUQ1b1x1_62898_LWUeeVYZ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.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-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits' -> 'wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits
WCS_IMAGE_NAME=wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits
WCS-calibrated image found: wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits
Checking if the catalog wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits.wcscat corresponding to the image wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits alredy exist and is non-empty...
Catalog wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits.wcscat corresponding to the image wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits
WCS catalog name: wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.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=1796, bad_region=0, passed=19819
Got 19819 stars (including 17995 good ones) from the SExtractor catalog wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits.wcscat
util/solve_plate_with_UCAC5 got 19819 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.7 to 59.4)
Done reading UCAC5 zone files...
Matched 4858 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4817 matched stars entering correct_measured_positions(), 4817 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4817 matched stars entering correct_measured_positions(), 19819 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.7 to 59.4)
Done reading UCAC5 zone files...
Matched 4858 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4817 matched stars entering correct_measured_positions(), 19819 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4817 matched stars entering correct_measured_positions(), 19819 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 4817 stars left (next iteration limit 5298)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits N_match=4817 sigma_overall_arcsec=0.341 sigma_q1_arcsec=0.431 sigma_q2_arcsec=0.350 sigma_q3_arcsec=0.327 sigma_q4_arcsec=0.289 n_q1=1188 n_q2=1031 n_q3=1236 n_q4=1362 worst_quadrant_to_overall_ratio=1.264
The image catalog is written to wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits -region wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.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.e4VCAyJVDG (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_2026-08-17_CI_Aur-01-Q1b1x1_022404_TTUQ1b1x1_62898_LWUeeVYZ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.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-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits' -> 'wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits
WCS_IMAGE_NAME=wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits
WCS-calibrated image found: wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits
Checking if the catalog wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits.wcscat corresponding to the image wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits alredy exist and is non-empty...
Catalog wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits.wcscat corresponding to the image wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits
WCS catalog name: wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.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=1769, bad_region=0, passed=19771
Got 19771 stars (including 17975 good ones) from the SExtractor catalog wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits.wcscat
util/solve_plate_with_UCAC5 got 19771 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.7 to 59.3)
Done reading UCAC5 zone files...
Matched 4856 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4817 matched stars entering correct_measured_positions(), 4817 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4817 matched stars entering correct_measured_positions(), 19771 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.7 to 59.3)
Done reading UCAC5 zone files...
Matched 4856 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4817 matched stars entering correct_measured_positions(), 19771 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 4817 matched stars entering correct_measured_positions(), 19771 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 4817 stars left (next iteration limit 5298)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits N_match=4817 sigma_overall_arcsec=0.354 sigma_q1_arcsec=0.445 sigma_q2_arcsec=0.356 sigma_q3_arcsec=0.341 sigma_q4_arcsec=0.305 n_q1=1191 n_q2=1033 n_q3=1224 n_q4=1369 worst_quadrant_to_overall_ratio=1.255
The image catalog is written to wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits -region wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.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.yz0P5KQHry (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_2026-08-17_CI_Aur-01-Q1b1x1_022404_TTUQ1b1x1_62898_LWUeeVYZ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Aur-01-Q1b1x1_022404_TTUQ1b1x1_62898_LWUeeVYZ/fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Aur-01-Q1b1x1_022404_TTUQ1b1x1_62898_LWUeeVYZ/fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Aur-01-Q1b1x1_022404_TTUQ1b1x1_62898_LWUeeVYZ/fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Aur-01-Q1b1x1_022404_TTUQ1b1x1_62898_LWUeeVYZ/fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Aur-01-Q1b1x1_022404_TTUQ1b1x1_62898_LWUeeVYZ/fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.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_2026-08-17_CI_Aur-01-Q1b1x1_022404_TTUQ1b1x1_62898_LWUeeVYZ/fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits
WCS_IMAGE_NAME=wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits
WCS-calibrated image found: wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits
Checking if the catalog wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits.wcscat corresponding to the image wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits.wcscat corresponding to the image wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Aur-01-Q1b1x1_022404_TTUQ1b1x1_62898_LWUeeVYZ/fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits
WCS catalog name: wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.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=110, bad_region=0, passed=3206
Got 3206 stars (including 3091 good ones) from the SExtractor catalog wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits.wcscat
util/solve_plate_with_UCAC5 got 3206 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 944.3'
Seting catalog search parameters based on the expected field of view 944.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013115 (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 0.010492 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.7 to 59.3)
Done reading UCAC5 zone files...
Matched 2990 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2956 matched stars entering correct_measured_positions(), 2952 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2956 matched stars entering correct_measured_positions(), 3201 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.7 to 59.3)
Done reading UCAC5 zone files...
Matched 2991 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2956 matched stars entering correct_measured_positions(), 3201 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 2956 matched stars entering correct_measured_positions(), 3201 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 2956 stars left (next iteration limit 3251)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=2956 robust_rms=7.622 arcsec worst_quadrant_rms=11.533 arcsec
SIP_REFIT: SIP order 3 trial: matched=2956 robust_rms=0.563 arcsec worst_quadrant_rms=0.716 arcsec
SIP_REFIT: SIP order 5 trial: matched=2956 robust_rms=0.452 arcsec worst_quadrant_rms=0.598 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=2956 robust_rms_before=1.300 arcsec robust_rms_before_corrected=0.450 arcsec robust_rms_after=0.452 arcsec worst_quadrant_rms_before=0.590 worst_quadrant_rms_after=0.598
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.590 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits N_match=2956 sigma_overall_arcsec=0.467 sigma_q1_arcsec=0.429 sigma_q2_arcsec=0.668 sigma_q3_arcsec=0.432 sigma_q4_arcsec=0.453 n_q1=1140 n_q2=496 n_q3=577 n_q4=743 worst_quadrant_to_overall_ratio=1.428
The image catalog is written to wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Aur-01-Q1b1x1_022404_TTUQ1b1x1_62898_LWUeeVYZ/fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits -region wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.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.GuDPDDQOcI (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_2026-08-17_CI_Aur-01-Q1b1x1_022404_TTUQ1b1x1_62898_LWUeeVYZ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Aur-01-Q1b1x1_022404_TTUQ1b1x1_62898_LWUeeVYZ/fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Aur-01-Q1b1x1_022404_TTUQ1b1x1_62898_LWUeeVYZ/fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Aur-01-Q1b1x1_022404_TTUQ1b1x1_62898_LWUeeVYZ/fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Aur-01-Q1b1x1_022404_TTUQ1b1x1_62898_LWUeeVYZ/fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Aur-01-Q1b1x1_022404_TTUQ1b1x1_62898_LWUeeVYZ/fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.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_2026-08-17_CI_Aur-01-Q1b1x1_022404_TTUQ1b1x1_62898_LWUeeVYZ/fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits
WCS_IMAGE_NAME=wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits
WCS-calibrated image found: wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits
Checking if the catalog wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits.wcscat corresponding to the image wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits.wcscat corresponding to the image wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Aur-01-Q1b1x1_022404_TTUQ1b1x1_62898_LWUeeVYZ/fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits
WCS catalog name: wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.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=104, bad_region=0, passed=3309
Got 3309 stars (including 3202 good ones) from the SExtractor catalog wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits.wcscat
util/solve_plate_with_UCAC5 got 3309 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 944.2'
Seting catalog search parameters based on the expected field of view 944.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013114 (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 0.010491 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.7 to 59.3)
Done reading UCAC5 zone files...
Matched 3094 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3057 matched stars entering correct_measured_positions(), 3056 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3057 matched stars entering correct_measured_positions(), 3308 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.7 to 59.3)
Done reading UCAC5 zone files...
Matched 3095 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 3058 matched stars entering correct_measured_positions(), 3308 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 3058 matched stars entering correct_measured_positions(), 3308 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 3058 stars left (next iteration limit 3362)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=3058 robust_rms=7.733 arcsec worst_quadrant_rms=11.757 arcsec
SIP_REFIT: SIP order 3 trial: matched=3058 robust_rms=0.561 arcsec worst_quadrant_rms=0.731 arcsec
SIP_REFIT: SIP order 5 trial: matched=3058 robust_rms=0.436 arcsec worst_quadrant_rms=0.546 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=3058 robust_rms_before=1.283 arcsec robust_rms_before_corrected=0.430 arcsec robust_rms_after=0.436 arcsec worst_quadrant_rms_before=0.540 worst_quadrant_rms_after=0.546
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.540 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits N_match=3058 sigma_overall_arcsec=0.431 sigma_q1_arcsec=0.411 sigma_q2_arcsec=0.581 sigma_q3_arcsec=0.416 sigma_q4_arcsec=0.408 n_q1=1227 n_q2=503 n_q3=567 n_q4=761 worst_quadrant_to_overall_ratio=1.347
The image catalog is written to wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Aur-01-Q1b1x1_022404_TTUQ1b1x1_62898_LWUeeVYZ/fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits -region wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Saving the final (post-refit) wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits to local_wcs_cache/
'wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits' -> 'local_wcs_cache/wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits'
Saving the final (post-refit) wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits to local_wcs_cache/
'wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits' -> 'local_wcs_cache/wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits'
Saving the final (post-refit) wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits to local_wcs_cache/
'wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits' -> 'local_wcs_cache/wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits'
Saving the final (post-refit) wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits to local_wcs_cache/
'wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits' -> 'local_wcs_cache/wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits sigma_overall=0.341 worst_q_ratio=1.264
ref2=Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits sigma_overall=0.354 worst_q_ratio=1.255
new1=fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits sigma_overall=0.467 worst_q_ratio=1.428
new2=fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits sigma_overall=0.431 worst_q_ratio=1.347
reference average sigma_overall=0.3475 worst_q_ratio=1.2595
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235_astrometric_residuals.png (4817 matched stars from wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.32 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236_astrometric_residuals.png (4817 matched stars from wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.32 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300_astrometric_residuals.png (2956 matched stars from wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.42 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301_astrometric_residuals.png (3058 matched stars from wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.40 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Aur-01-Q1b1x1_022404_TTUQ1b1x1_62898_LWUeeVYZ/wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits'
Saving fully-calibrated image wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Aur-01-Q1b1x1_022404_TTUQ1b1x1_62898_LWUeeVYZ/wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits'
Preparing the HTML report for the field Aur-01-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Aur-01-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 ####
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-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Aur-01-Q1b1x1_022404_TTUQ1b1x1_62898_LWUeeVYZ/fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Aur-01-Q1b1x1_022404_TTUQ1b1x1_62898_LWUeeVYZ/fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits
SExtractor catalog cache: saved Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits.cat to cache
SExtractor catalog cache: saved Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.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-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Aur-01-Q1b1x1_022404_TTUQ1b1x1_62898_LWUeeVYZ/fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Aur-01-Q1b1x1_022404_TTUQ1b1x1_62898_LWUeeVYZ/fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits
Creating symlink local_wcs_cache/wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits
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-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits exists and is non-empty
wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits exists and is non-empty
wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits exists and is non-empty
wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits (1st reference image)
verification OK: wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits
Image size: 941.7'x627.2' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:38:52.744 +53:59:24.28 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-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits (1st new image)
verification OK: wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits
Image size: 944.3'x627.0' 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: 05:38:47.497 +53:58:50.52 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:38:52.744 +53:59:24.28
Second-epoch image center 05:38:47.497 +53:58:50.52
Angular distance between the image centers 0.0159 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits (2nd new image)
verification OK: wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits
Image size: 944.2'x627.0' 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: 05:38:45.550 +53:59:23.35 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:38:52.744 +53:59:24.28
Second-epoch image center 05:38:45.550 +53:59:23.35
Angular distance between the image centers 0.0176 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 05:38:47.497 +53:58:50.52
Second-epoch second image center 05:38:45.550 +53:59:23.35
Angular distance between the image centers 0.01029 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-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits &> /tmp/tmp.JZkLEs1FW0
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits &> /tmp/tmp.tvHx1VNhkw
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Aur-01-Q1b1x1_022404_TTUQ1b1x1_62898_LWUeeVYZ/fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits &> /tmp/tmp.oME8sFeA26
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Aur-01-Q1b1x1_022404_TTUQ1b1x1_62898_LWUeeVYZ/fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Aur-01-Q1b1x1_022404_TTUQ1b1x1_62898_LWUeeVYZ/fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits &> /tmp/tmp.c5yEMgOi5F
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Aur-01-Q1b1x1_022404_TTUQ1b1x1_62898_LWUeeVYZ/fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.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-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits and wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.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-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits and wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits.wcscat
Found non-empty wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits and wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits.wcscat
The reference image (wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits) and catalog (wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits.wcscat) found
'wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits.wcscat' -> 'wcsmag.cat'
Read 142069 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 70.1251 to 100.1985 deg, Dec +47.6928 to +59.3619 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 70.1251 to 100.1985 deg, Dec 47.6928 to 59.3619 deg
Loaded 11744 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): 6276 out of 8345 total matches.
Matched with Tycho-2 8345 out of 142069 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.773000
a=0.000000 b=1.000000 c=22.773000
From vast_summary.log: estimated ref. image limiting mag.: -7.26
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.51
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.51
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 142069 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 70.1251 to 100.1985 deg, Dec +47.6928 to +59.3619 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 70.1251 to 100.1985 deg, Dec 47.6928 to 59.3619 deg
Loaded 11744 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): 6276 out of 8345 total matches.
Matched with Tycho-2 8345 out of 142069 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits
Forced-photometry filter: calibrated wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits -> calib.txt_param_ref_wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits (aperture=4.7)
Read 142378 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 70.1601 to 100.1988 deg, Dec +47.6936 to +59.3541 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 70.1601 to 100.1988 deg, Dec 47.6936 to 59.3541 deg
Loaded 11720 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): 6294 out of 8348 total matches.
Matched with Tycho-2 8348 out of 142378 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits
Forced-photometry filter: calibrated wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits -> calib.txt_param_ref_wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits (aperture=4.7)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 123 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits
2.0 pix Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits
2.4 pix fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits
2.4 pix fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits
Limiting magnitude estimates:
15.5 mag. Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits
15.5 mag. Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits
13.2 mag. fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits
13.3 mag. fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits
All-image limiting magnitude estimate: 13.2 (SNR ) 12.9 (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.JZkLEs1FW0 (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_2026-08-17_CI_Aur-01-Q1b1x1_022404_TTUQ1b1x1_62898_LWUeeVYZ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.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-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits' -> 'wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits
WCS_IMAGE_NAME=wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits
WCS-calibrated image found: wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits
Checking if the catalog wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits.wcscat corresponding to the image wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits alredy exist and is non-empty...
Catalog wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits.wcscat corresponding to the image wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits
WCS catalog name: wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.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=40, blended=15126, bad_region=1, passed=142029
Got 142029 stars (including 126648 good ones) from the SExtractor catalog wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits.wcscat
util/solve_plate_with_UCAC5 got 142029 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.7 to 59.4)
Done reading UCAC5 zone files...
Matched 4856 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4837 matched stars entering correct_measured_positions(), 4837 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4837 matched stars entering correct_measured_positions(), 142029 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.7 to 59.4)
Done reading UCAC5 zone files...
Matched 4857 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4835 matched stars entering correct_measured_positions(), 142029 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 4835 matched stars entering correct_measured_positions(), 142029 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 4835 stars left (next iteration limit 5320)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits N_match=4835 sigma_overall_arcsec=0.329 sigma_q1_arcsec=0.401 sigma_q2_arcsec=0.336 sigma_q3_arcsec=0.311 sigma_q4_arcsec=0.282 n_q1=1195 n_q2=1063 n_q3=1229 n_q4=1348 worst_quadrant_to_overall_ratio=1.218
The image catalog is written to wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits -region wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.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.tvHx1VNhkw (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_2026-08-17_CI_Aur-01-Q1b1x1_022404_TTUQ1b1x1_62898_LWUeeVYZ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.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-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits' -> 'wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits
WCS_IMAGE_NAME=wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits
WCS-calibrated image found: wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits
Checking if the catalog wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits.wcscat corresponding to the image wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits alredy exist and is non-empty...
Catalog wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits.wcscat corresponding to the image wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits
WCS catalog name: wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.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=45, blended=15255, bad_region=2, passed=142333
Got 142333 stars (including 126844 good ones) from the SExtractor catalog wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits.wcscat
util/solve_plate_with_UCAC5 got 142333 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.7 to 59.4)
Done reading UCAC5 zone files...
Matched 4857 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4839 matched stars entering correct_measured_positions(), 4839 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4839 matched stars entering correct_measured_positions(), 142333 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.7 to 59.4)
Done reading UCAC5 zone files...
Matched 4857 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4838 matched stars entering correct_measured_positions(), 142333 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4838 matched stars entering correct_measured_positions(), 142333 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 4838 stars left (next iteration limit 5322)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits N_match=4838 sigma_overall_arcsec=0.339 sigma_q1_arcsec=0.406 sigma_q2_arcsec=0.350 sigma_q3_arcsec=0.329 sigma_q4_arcsec=0.294 n_q1=1190 n_q2=1053 n_q3=1236 n_q4=1359 worst_quadrant_to_overall_ratio=1.196
The image catalog is written to wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits -region wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.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.oME8sFeA26 (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_2026-08-17_CI_Aur-01-Q1b1x1_022404_TTUQ1b1x1_62898_LWUeeVYZ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Aur-01-Q1b1x1_022404_TTUQ1b1x1_62898_LWUeeVYZ/fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Aur-01-Q1b1x1_022404_TTUQ1b1x1_62898_LWUeeVYZ/fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Aur-01-Q1b1x1_022404_TTUQ1b1x1_62898_LWUeeVYZ/fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Aur-01-Q1b1x1_022404_TTUQ1b1x1_62898_LWUeeVYZ/fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Aur-01-Q1b1x1_022404_TTUQ1b1x1_62898_LWUeeVYZ/fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.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_2026-08-17_CI_Aur-01-Q1b1x1_022404_TTUQ1b1x1_62898_LWUeeVYZ/fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits
WCS_IMAGE_NAME=wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits
WCS-calibrated image found: wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits
Checking if the catalog wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits.wcscat corresponding to the image wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits.wcscat corresponding to the image wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Aur-01-Q1b1x1_022404_TTUQ1b1x1_62898_LWUeeVYZ/fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits
WCS catalog name: wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.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=721, bad_region=26, passed=28390
Got 28390 stars (including 27591 good ones) from the SExtractor catalog wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits.wcscat
util/solve_plate_with_UCAC5 got 28390 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 944.3'
Seting catalog search parameters based on the expected field of view 944.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013115 (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 0.010492 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.7 to 59.3)
Done reading UCAC5 zone files...
Matched 4857 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4808 matched stars entering correct_measured_positions(), 4807 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4808 matched stars entering correct_measured_positions(), 28388 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.7 to 59.3)
Done reading UCAC5 zone files...
Matched 4857 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4807 matched stars entering correct_measured_positions(), 28389 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 4807 matched stars entering correct_measured_positions(), 28389 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 4807 stars left (next iteration limit 5288)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4807 robust_rms=7.260 arcsec worst_quadrant_rms=10.938 arcsec
SIP_REFIT: SIP order 3 trial: matched=4807 robust_rms=0.592 arcsec worst_quadrant_rms=0.720 arcsec
SIP_REFIT: SIP order 5 trial: matched=4807 robust_rms=0.477 arcsec worst_quadrant_rms=0.614 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4807 robust_rms_before=1.302 arcsec robust_rms_before_corrected=0.458 arcsec robust_rms_after=0.477 arcsec worst_quadrant_rms_before=0.574 worst_quadrant_rms_after=0.614
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.574 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits N_match=4807 sigma_overall_arcsec=0.453 sigma_q1_arcsec=0.440 sigma_q2_arcsec=0.611 sigma_q3_arcsec=0.407 sigma_q4_arcsec=0.435 n_q1=1851 n_q2=767 n_q3=991 n_q4=1198 worst_quadrant_to_overall_ratio=1.347
The image catalog is written to wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Aur-01-Q1b1x1_022404_TTUQ1b1x1_62898_LWUeeVYZ/fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits -region wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.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.c5yEMgOi5F (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_2026-08-17_CI_Aur-01-Q1b1x1_022404_TTUQ1b1x1_62898_LWUeeVYZ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Aur-01-Q1b1x1_022404_TTUQ1b1x1_62898_LWUeeVYZ/fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Aur-01-Q1b1x1_022404_TTUQ1b1x1_62898_LWUeeVYZ/fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Aur-01-Q1b1x1_022404_TTUQ1b1x1_62898_LWUeeVYZ/fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Aur-01-Q1b1x1_022404_TTUQ1b1x1_62898_LWUeeVYZ/fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Aur-01-Q1b1x1_022404_TTUQ1b1x1_62898_LWUeeVYZ/fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.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_2026-08-17_CI_Aur-01-Q1b1x1_022404_TTUQ1b1x1_62898_LWUeeVYZ/fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits
WCS_IMAGE_NAME=wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits
WCS-calibrated image found: wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits
Checking if the catalog wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits.wcscat corresponding to the image wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits.wcscat corresponding to the image wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Aur-01-Q1b1x1_022404_TTUQ1b1x1_62898_LWUeeVYZ/fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits
WCS catalog name: wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=799, bad_region=30, passed=29241
Got 29241 stars (including 28360 good ones) from the SExtractor catalog wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits.wcscat
util/solve_plate_with_UCAC5 got 29241 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 944.2'
Seting catalog search parameters based on the expected field of view 944.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013114 (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 0.010491 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.7 to 59.3)
Done reading UCAC5 zone files...
Matched 4853 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4803 matched stars entering correct_measured_positions(), 4802 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4803 matched stars entering correct_measured_positions(), 29222 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.7 to 59.3)
Done reading UCAC5 zone files...
Matched 4852 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4803 matched stars entering correct_measured_positions(), 29222 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 4803 matched stars entering correct_measured_positions(), 29222 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 4803 stars left (next iteration limit 5283)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4803 robust_rms=7.250 arcsec worst_quadrant_rms=10.939 arcsec
SIP_REFIT: SIP order 3 trial: matched=4803 robust_rms=0.571 arcsec worst_quadrant_rms=0.778 arcsec
SIP_REFIT: SIP order 5 trial: matched=4803 robust_rms=0.461 arcsec worst_quadrant_rms=0.570 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4803 robust_rms_before=1.280 arcsec robust_rms_before_corrected=0.427 arcsec robust_rms_after=0.461 arcsec worst_quadrant_rms_before=0.509 worst_quadrant_rms_after=0.570
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.509 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits N_match=4803 sigma_overall_arcsec=0.424 sigma_q1_arcsec=0.423 sigma_q2_arcsec=0.542 sigma_q3_arcsec=0.397 sigma_q4_arcsec=0.401 n_q1=1884 n_q2=733 n_q3=974 n_q4=1212 worst_quadrant_to_overall_ratio=1.278
The image catalog is written to wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Aur-01-Q1b1x1_022404_TTUQ1b1x1_62898_LWUeeVYZ/fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits -region wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.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-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.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_2026-08-17_CI_Aur-01-Q1b1x1_022404_TTUQ1b1x1_62898_LWUeeVYZ/wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-22-19_20.00sec_-0.00C_LIGHTs_0300.fits
Saving fully-calibrated image wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.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_2026-08-17_CI_Aur-01-Q1b1x1_022404_TTUQ1b1x1_62898_LWUeeVYZ/wcs_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301.fits
Preparing the HTML report for the field Aur-01-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 06:13:57.95 +51:59:26.7: 12.35 +/- 0.01 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:48:43.79 +56:48:47.9: 12.43 +/- 0.01 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:19:15.72 +56:20:25.5: 12.55 +/- 0.01 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:15:20.29 +49:48:50.1: 12.15 +/- 0.01 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:40:31.23 +55:06:37.2: 12.55 +/- 0.01 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 06:13:57.95 +51:59:26.7: 12.32 +/- 0.01 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:19:15.72 +56:20:25.5: 12.56 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.34 +/- 0.01
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:48:43.79 +56:48:47.9: 12.44 +/- 0.01 detection
Forced photometry filter REJECTED candidate at 06:13:57.95 +51:59:26.7: ref_mag=12.34 +/- 0.01 new_mean_mag=12.6289 delta=-0.29 (need > 0.90)
Forced photometry reference-image weighted average: 12.55 +/- 0.01
Forced photometry filter REJECTED candidate at 05:19:15.72 +56:20:25.5: ref_mag=12.55 +/- 0.01 new_mean_mag=12.5864 delta=-0.04 (need > 0.90)
Forced photometry reference-image weighted average: 12.43 +/- 0.01
Forced photometry filter REJECTED candidate at 05:48:43.79 +56:48:47.9: ref_mag=12.43 +/- 0.01 new_mean_mag=12.0387 delta=0.39 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:15:20.29 +49:48:50.1: 12.12 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.13 +/- 0.01
Forced photometry filter REJECTED candidate at 05:15:20.29 +49:48:50.1: ref_mag=12.13 +/- 0.01 new_mean_mag=12.4874 delta=-0.35 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:40:31.23 +55:06:37.2: 12.54 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.55 +/- 0.01
Forced photometry filter REJECTED candidate at 05:40:31.23 +55:06:37.2: ref_mag=12.55 +/- 0.01 new_mean_mag=12.0023 delta=0.55 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:43:19.75 +52:30:09.3: 12.81 +/- 0.02 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:32:02.93 +51:15:06.7: 12.93 +/- 0.02 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:26:44.27 +56:22:27.5: 12.79 +/- 0.02 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:27:32.38 +53:45:09.5: 12.98 +/- 0.02 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:43:19.75 +52:30:09.3: 12.83 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.01
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:32:02.93 +51:15:06.7: 12.89 +/- 0.02 detection
Forced photometry filter REJECTED candidate at 05:43:19.75 +52:30:09.3: ref_mag=12.82 +/- 0.01 new_mean_mag=12.4008 delta=0.42 (need > 0.90)
Forced photometry reference-image weighted average: 12.91 +/- 0.02
Forced photometry filter REJECTED candidate at 05:32:02.93 +51:15:06.7: ref_mag=12.91 +/- 0.02 new_mean_mag=12.2713 delta=0.64 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:39:19.04 +56:04:17.3: 13.21 +/- 0.03 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:26:44.27 +56:22:27.5: 12.76 +/- 0.02 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:27:32.38 +53:45:09.5: 12.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.01
Forced photometry filter REJECTED candidate at 05:26:44.27 +56:22:27.5: ref_mag=12.78 +/- 0.01 new_mean_mag=12.5531 delta=0.22 (need > 0.90)
Forced photometry reference-image weighted average: 12.98 +/- 0.02
Forced photometry filter REJECTED candidate at 05:27:32.38 +53:45:09.5: ref_mag=12.98 +/- 0.02 new_mean_mag=12.4803 delta=0.49 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:39:19.04 +56:04:17.3: 13.22 +/- 0.03 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:22:37.79 +51:12:33.9: 13.39 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:25:08.77 +55:23:47.8: 13.12 +/- 0.02 detection
Forced photometry filter REJECTED candidate at 05:39:19.04 +56:04:17.3: ref_mag=13.21 +/- 0.02 new_mean_mag=12.5909 delta=0.62 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:37:06.93 +56:04:06.1: 13.50 +/- 0.04 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:33:54.75 +52:34:08.6: 13.90 +/- 0.05 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:25:08.77 +55:23:47.8: 13.09 +/- 0.02 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:22:37.79 +51:12:33.9: 13.38 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.02
Forced photometry filter REJECTED candidate at 05:25:08.77 +55:23:47.8: ref_mag=13.10 +/- 0.02 new_mean_mag=12.8382 delta=0.26 (need > 0.90)
Forced photometry reference-image weighted average: 13.39 +/- 0.02
Forced photometry filter REJECTED candidate at 05:22:37.79 +51:12:33.9: ref_mag=13.39 +/- 0.02 new_mean_mag=12.7833 delta=0.60 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:37:06.93 +56:04:06.1: 13.47 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.03
Forced photometry filter REJECTED candidate at 05:37:06.93 +56:04:06.1: ref_mag=13.49 +/- 0.03 new_mean_mag=12.8522 delta=0.63 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:33:54.75 +52:34:08.6: 14.00 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.95 +/- 0.04
Forced photometry filter REJECTED candidate at 05:33:54.75 +52:34:08.6: ref_mag=13.95 +/- 0.04 new_mean_mag=13.2839 delta=0.66 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:50:19.24 +56:29:05.9: 13.29 +/- 0.03 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:29:54.09 +52:31:33.7: 13.42 +/- 0.03 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:43:02.29 +56:26:26.1: 13.78 +/- 0.04 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:53:22.42 +56:57:07.2: 13.53 +/- 0.03 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 04:54:24.73 +50:50:08.6: 13.89 +/- 0.06 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:50:19.24 +56:29:05.9: 13.36 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.02
Forced photometry filter KEPT candidate at 05:50:19.24 +56:29:05.9: ref_mag=13.33 +/- 0.02 new_mean_mag=12.3624 delta=0.96 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:29:54.09 +52:31:33.7: 13.44 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.02
Forced photometry filter KEPT candidate at 05:29:54.09 +52:31:33.7: ref_mag=13.43 +/- 0.02 new_mean_mag=12.5033 delta=0.92 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:34:52.94 +51:53:03.7: 13.85 +/- 0.04 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:44:15.90 +55:09:50.1: 13.88 +/- 0.04 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:43:02.29 +56:26:26.1: 13.85 +/- 0.05 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:53:22.42 +56:57:07.2: 13.49 +/- 0.03 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 06:01:21.71 +57:12:11.1: 13.85 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.02
Forced photometry reference-image weighted average: 13.81 +/- 0.03
Forced photometry filter KEPT candidate at 05:43:02.29 +56:26:26.1: ref_mag=13.81 +/- 0.03 new_mean_mag=12.8294 delta=0.98 (need > 0.90)
Forced photometry filter KEPT candidate at 05:53:22.42 +56:57:07.2: ref_mag=13.51 +/- 0.02 new_mean_mag=12.5981 delta=0.91 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 04:54:24.73 +50:50:08.6: 13.91 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.90 +/- 0.04
Forced photometry filter KEPT candidate at 04:54:24.73 +50:50:08.6: ref_mag=13.90 +/- 0.04 new_mean_mag=12.7474 delta=1.15 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:47:18.83 +55:50:29.5: 13.87 +/- 0.05 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:44:15.90 +55:09:50.1: 13.71 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.77 +/- 0.03
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:34:52.94 +51:53:03.7: 13.85 +/- 0.04 detection
Forced photometry filter KEPT candidate at 05:44:15.90 +55:09:50.1: ref_mag=13.77 +/- 0.03 new_mean_mag=12.8067 delta=0.96 (need > 0.90)
Forced photometry reference-image weighted average: 13.85 +/- 0.03
Forced photometry filter KEPT candidate at 05:34:52.94 +51:53:03.7: ref_mag=13.85 +/- 0.03 new_mean_mag=12.8149 delta=1.04 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 06:01:21.71 +57:12:11.1: 13.95 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.90 +/- 0.03
Forced photometry filter KEPT candidate at 06:01:21.71 +57:12:11.1: ref_mag=13.90 +/- 0.03 new_mean_mag=12.8104 delta=1.09 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:34:58.07 +53:25:58.2: 13.83 +/- 0.05 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:47:18.83 +55:50:29.5: 13.84 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.85 +/- 0.03
Forced photometry filter KEPT candidate at 05:47:18.83 +55:50:29.5: ref_mag=13.85 +/- 0.03 new_mean_mag=12.8234 delta=1.03 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:34:58.07 +53:25:58.2: 13.77 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.80 +/- 0.03
Forced photometry filter KEPT candidate at 05:34:58.07 +53:25:58.2: ref_mag=13.80 +/- 0.03 new_mean_mag=12.8079 delta=0.99 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:40:38.78 +53:24:10.7: 13.82 +/- 0.04 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:40:38.78 +53:24:10.7: 13.82 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.82 +/- 0.03
Forced photometry filter KEPT candidate at 05:40:38.78 +53:24:10.7: ref_mag=13.82 +/- 0.03 new_mean_mag=12.8134 delta=1.01 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 04:57:45.79 +51:36:13.2: 13.83 +/- 0.05 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 04:57:45.79 +51:36:13.2: 13.79 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.03
Forced photometry filter KEPT candidate at 04:57:45.79 +51:36:13.2: ref_mag=13.81 +/- 0.03 new_mean_mag=12.7459 delta=1.06 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:54:47.45 +57:19:44.9: 13.82 +/- 0.05 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:54:47.45 +57:19:44.9: 13.92 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.87 +/- 0.04
Forced photometry filter KEPT candidate at 05:54:47.45 +57:19:44.9: ref_mag=13.87 +/- 0.04 new_mean_mag=12.8335 delta=1.03 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:32:47.75 +50:53:24.3: 13.80 +/- 0.04 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:32:47.75 +50:53:24.3: 13.79 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.80 +/- 0.03
Forced photometry filter KEPT candidate at 05:32:47.75 +50:53:24.3: ref_mag=13.80 +/- 0.03 new_mean_mag=12.7515 delta=1.04 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:50:02.10 +56:08:33.1: 13.80 +/- 0.04 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:50:02.10 +56:08:33.1: 13.82 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.03
Forced photometry filter KEPT candidate at 05:50:02.10 +56:08:33.1: ref_mag=13.81 +/- 0.03 new_mean_mag=12.8071 delta=1.00 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:40:14.81 +54:02:48.2: 13.78 +/- 0.04 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:40:14.81 +54:02:48.2: 13.71 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.74 +/- 0.03
Forced photometry filter KEPT candidate at 05:40:14.81 +54:02:48.2: ref_mag=13.74 +/- 0.03 new_mean_mag=12.8272 delta=0.91 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:39:37.99 +54:33:15.3: 13.76 +/- 0.03 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:37:53.88 +53:58:59.9: 13.77 +/- 0.04 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:39:37.99 +54:33:15.3: 13.81 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.78 +/- 0.03
Forced photometry filter KEPT candidate at 05:39:37.99 +54:33:15.3: ref_mag=13.78 +/- 0.03 new_mean_mag=12.8068 delta=0.98 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:37:53.88 +53:58:59.9: 13.75 +/- 0.04 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:31:42.82 +52:59:28.1: 13.74 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.76 +/- 0.03
Forced photometry filter KEPT candidate at 05:37:53.88 +53:58:59.9: ref_mag=13.76 +/- 0.03 new_mean_mag=12.7125 delta=1.05 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:26:53.09 +51:50:32.7: 13.78 +/- 0.04 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:31:42.82 +52:59:28.1: 13.76 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.75 +/- 0.03
Forced photometry filter KEPT candidate at 05:31:42.82 +52:59:28.1: ref_mag=13.75 +/- 0.03 new_mean_mag=12.8265 delta=0.92 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:26:53.09 +51:50:32.7: 13.72 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.75 +/- 0.03
Forced photometry filter KEPT candidate at 05:26:53.09 +51:50:32.7: ref_mag=13.75 +/- 0.03 new_mean_mag=12.8110 delta=0.94 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:38:46.03 +52:40:16.0: 13.72 +/- 0.03 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:41:29.43 +54:38:58.8: 13.76 +/- 0.04 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:38:46.03 +52:40:16.0: 13.71 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.02
Forced photometry filter KEPT candidate at 05:38:46.03 +52:40:16.0: ref_mag=13.71 +/- 0.02 new_mean_mag=12.7814 delta=0.93 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:41:29.43 +54:38:58.8: 13.77 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.77 +/- 0.03
Forced photometry filter KEPT candidate at 05:41:29.43 +54:38:58.8: ref_mag=13.77 +/- 0.03 new_mean_mag=12.8057 delta=0.96 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:40:15.14 +54:17:29.3: 13.72 +/- 0.04 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:40:15.14 +54:17:29.3: 13.65 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.03
Forced photometry filter KEPT candidate at 05:40:15.14 +54:17:29.3: ref_mag=13.68 +/- 0.03 new_mean_mag=12.7001 delta=0.98 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:50:07.59 +56:13:10.7: 13.71 +/- 0.04 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:50:07.59 +56:13:10.7: 13.72 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.72 +/- 0.03
Forced photometry filter KEPT candidate at 05:50:07.59 +56:13:10.7: ref_mag=13.72 +/- 0.03 new_mean_mag=12.7669 delta=0.95 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:32:04.11 +50:32:36.9: 13.74 +/- 0.04 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:32:04.11 +50:32:36.9: 13.74 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.74 +/- 0.03
Forced photometry filter KEPT candidate at 05:32:04.11 +50:32:36.9: ref_mag=13.74 +/- 0.03 new_mean_mag=12.7799 delta=0.96 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:43:20.94 +53:14:52.8: 13.71 +/- 0.04 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:43:20.94 +53:14:52.8: 13.70 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.70 +/- 0.03
Forced photometry filter KEPT candidate at 05:43:20.94 +53:14:52.8: ref_mag=13.70 +/- 0.03 new_mean_mag=12.7829 delta=0.92 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 04:57:46.41 +50:25:34.1: 13.70 +/- 0.05 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 04:57:46.41 +50:25:34.1: 13.67 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.03
Forced photometry filter KEPT candidate at 04:57:46.41 +50:25:34.1: ref_mag=13.68 +/- 0.03 new_mean_mag=12.7315 delta=0.95 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:53:27.12 +57:10:27.0: 13.72 +/- 0.04 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:35:32.95 +53:53:37.0: 13.68 +/- 0.03 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:53:27.12 +57:10:27.0: 13.64 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.03
Forced photometry filter KEPT candidate at 05:53:27.12 +57:10:27.0: ref_mag=13.67 +/- 0.03 new_mean_mag=12.6558 delta=1.02 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:44:05.84 +55:40:28.7: 13.69 +/- 0.04 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:20:36.38 +49:48:13.2: 13.70 +/- 0.04 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:07:34.64 +49:24:22.7: 13.66 +/- 0.04 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:35:32.95 +53:53:37.0: 13.71 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.70 +/- 0.02
Forced photometry filter KEPT candidate at 05:35:32.95 +53:53:37.0: ref_mag=13.70 +/- 0.02 new_mean_mag=12.6737 delta=1.02 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:44:05.84 +55:40:28.7: 13.70 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.69 +/- 0.03
Forced photometry filter KEPT candidate at 05:44:05.84 +55:40:28.7: ref_mag=13.69 +/- 0.03 new_mean_mag=12.7398 delta=0.95 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:07:34.64 +49:24:22.7: 13.59 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.03
Forced photometry filter KEPT candidate at 05:07:34.64 +49:24:22.7: ref_mag=13.62 +/- 0.03 new_mean_mag=12.7054 delta=0.92 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:20:36.38 +49:48:13.2: 13.73 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.03
Forced photometry filter KEPT candidate at 05:20:36.38 +49:48:13.2: ref_mag=13.71 +/- 0.03 new_mean_mag=12.7638 delta=0.95 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:46:04.02 +55:39:55.4: 13.63 +/- 0.04 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:46:04.02 +55:39:55.4: 13.63 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.63 +/- 0.02
Forced photometry filter KEPT candidate at 05:46:04.02 +55:39:55.4: ref_mag=13.63 +/- 0.02 new_mean_mag=12.6752 delta=0.95 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:42:54.04 +54:52:53.3: 13.63 +/- 0.03 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:42:54.04 +54:52:53.3: 13.56 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.02
Forced photometry filter KEPT candidate at 05:42:54.04 +54:52:53.3: ref_mag=13.59 +/- 0.02 new_mean_mag=12.6874 delta=0.91 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:52:07.90 +56:52:53.8: 13.64 +/- 0.04 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:52:07.90 +56:52:53.8: 13.59 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.03
Forced photometry filter KEPT candidate at 05:52:07.90 +56:52:53.8: ref_mag=13.61 +/- 0.03 new_mean_mag=12.7092 delta=0.90 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:38:55.51 +55:58:52.7: 13.62 +/- 0.03 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:38:55.51 +55:58:52.7: 13.57 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.02
Forced photometry filter KEPT candidate at 05:38:55.51 +55:58:52.7: ref_mag=13.60 +/- 0.02 new_mean_mag=12.5824 delta=1.02 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:35:22.99 +53:16:01.5: 13.60 +/- 0.03 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:35:22.99 +53:16:01.5: 13.61 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.02
Forced photometry filter KEPT candidate at 05:35:22.99 +53:16:01.5: ref_mag=13.61 +/- 0.02 new_mean_mag=12.6858 delta=0.92 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:35:41.59 +53:53:29.7: 13.58 +/- 0.03 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:35:41.59 +53:53:29.7: 13.69 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.63 +/- 0.02
Forced photometry filter KEPT candidate at 05:35:41.59 +53:53:29.7: ref_mag=13.63 +/- 0.02 new_mean_mag=12.6289 delta=1.01 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:41:05.59 +54:34:29.4: 13.58 +/- 0.03 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:41:05.59 +54:34:29.4: 13.63 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.02
Forced photometry filter KEPT candidate at 05:41:05.59 +54:34:29.4: ref_mag=13.61 +/- 0.02 new_mean_mag=12.6691 delta=0.94 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:43:16.88 +55:14:46.9: 13.57 +/- 0.03 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:46:54.01 +55:50:01.2: 13.54 +/- 0.03 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:43:16.88 +55:14:46.9: 13.57 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.02
Forced photometry filter KEPT candidate at 05:43:16.88 +55:14:46.9: ref_mag=13.57 +/- 0.02 new_mean_mag=12.6574 delta=0.91 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:36:56.31 +55:28:23.8: 13.26 +/- 0.02 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:46:54.01 +55:50:01.2: 13.53 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.54 +/- 0.02
Forced photometry filter KEPT candidate at 05:46:54.01 +55:50:01.2: ref_mag=13.54 +/- 0.02 new_mean_mag=12.5397 delta=1.00 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:36:56.31 +55:28:23.8: 13.29 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.02
Forced photometry filter REJECTED candidate at 05:36:56.31 +55:28:23.8: ref_mag=13.28 +/- 0.02 new_mean_mag=12.5624 delta=0.71 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 06:02:54.74 +57:40:37.8: 13.52 +/- 0.04 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:55:06.04 +57:07:01.8: 13.48 +/- 0.03 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:42:46.09 +54:44:39.6: 13.48 +/- 0.03 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:55:06.04 +57:07:01.8: 13.50 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.02
Forced photometry filter KEPT candidate at 05:55:06.04 +57:07:01.8: ref_mag=13.49 +/- 0.02 new_mean_mag=12.5503 delta=0.94 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 06:02:54.74 +57:40:37.8: 13.53 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.52 +/- 0.03
Forced photometry filter KEPT candidate at 06:02:54.74 +57:40:37.8: ref_mag=13.52 +/- 0.03 new_mean_mag=12.5690 delta=0.95 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:42:46.09 +54:44:39.6: 13.44 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.02
Forced photometry filter KEPT candidate at 05:42:46.09 +54:44:39.6: ref_mag=13.46 +/- 0.02 new_mean_mag=12.5308 delta=0.93 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 06:03:34.05 +57:50:33.0: 13.48 +/- 0.03 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 06:03:34.05 +57:50:33.0: 13.43 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.02
Forced photometry filter KEPT candidate at 06:03:34.05 +57:50:33.0: ref_mag=13.45 +/- 0.02 new_mean_mag=12.5240 delta=0.93 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:35:01.42 +54:18:43.4: 13.46 +/- 0.03 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:35:01.42 +54:18:43.4: 13.47 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.02
Forced photometry filter KEPT candidate at 05:35:01.42 +54:18:43.4: ref_mag=13.47 +/- 0.02 new_mean_mag=12.4796 delta=0.99 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:57:39.19 +57:38:03.1: 13.44 +/- 0.03 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:57:39.19 +57:38:03.1: 13.55 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.02
Forced photometry filter KEPT candidate at 05:57:39.19 +57:38:03.1: ref_mag=13.49 +/- 0.02 new_mean_mag=12.4951 delta=1.00 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:44:34.08 +55:34:38.1: 13.06 +/- 0.02 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:44:34.08 +55:34:38.1: 13.07 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.01
Forced photometry filter REJECTED candidate at 05:44:34.08 +55:34:38.1: ref_mag=13.07 +/- 0.01 new_mean_mag=12.2585 delta=0.81 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 06:04:24.29 +58:22:52.0: 13.43 +/- 0.03 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:40:22.07 +55:45:24.0: 13.40 +/- 0.03 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 06:04:24.29 +58:22:52.0: 13.44 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.02
Forced photometry filter KEPT candidate at 06:04:24.29 +58:22:52.0: ref_mag=13.43 +/- 0.02 new_mean_mag=12.4465 delta=0.99 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:40:22.07 +55:45:24.0: 13.39 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.02
Forced photometry filter KEPT candidate at 05:40:22.07 +55:45:24.0: ref_mag=13.40 +/- 0.02 new_mean_mag=12.4098 delta=0.99 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:42:40.50 +56:20:38.0: 13.39 +/- 0.03 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:42:40.50 +56:20:38.0: 13.46 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.02
Forced photometry filter KEPT candidate at 05:42:40.50 +56:20:38.0: ref_mag=13.42 +/- 0.02 new_mean_mag=12.4773 delta=0.94 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:57:54.51 +57:21:52.1: 13.39 +/- 0.03 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:57:54.51 +57:21:52.1: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.02
Forced photometry filter KEPT candidate at 05:57:54.51 +57:21:52.1: ref_mag=13.39 +/- 0.02 new_mean_mag=12.4410 delta=0.95 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:26:01.58 +51:33:53.2: 13.40 +/- 0.03 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:26:01.58 +51:33:53.2: 13.49 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.02
Forced photometry filter KEPT candidate at 05:26:01.58 +51:33:53.2: ref_mag=13.44 +/- 0.02 new_mean_mag=12.4978 delta=0.94 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:34:17.21 +51:20:54.3: 13.28 +/- 0.02 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 06:02:41.20 +58:29:42.4: 13.25 +/- 0.03 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:34:17.21 +51:20:54.3: 13.32 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.02
Forced photometry filter KEPT candidate at 05:34:17.21 +51:20:54.3: ref_mag=13.30 +/- 0.02 new_mean_mag=12.3358 delta=0.96 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 06:02:41.20 +58:29:42.4: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.02
Forced photometry filter KEPT candidate at 06:02:41.20 +58:29:42.4: ref_mag=13.27 +/- 0.02 new_mean_mag=12.3336 delta=0.94 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:55:36.78 +56:56:53.1: 13.01 +/- 0.02 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:55:36.78 +56:56:53.1: 13.02 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.02
Forced photometry filter REJECTED candidate at 05:55:36.78 +56:56:53.1: ref_mag=13.01 +/- 0.02 new_mean_mag=12.2088 delta=0.81 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:38:32.79 +53:39:11.5: 13.11 +/- 0.02 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:42:37.11 +55:26:33.0: 13.06 +/- 0.02 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:38:32.79 +53:39:11.5: 13.16 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.02
Forced photometry filter KEPT candidate at 05:38:32.79 +53:39:11.5: ref_mag=13.13 +/- 0.02 new_mean_mag=12.1263 delta=1.00 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:42:37.11 +55:26:33.0: 13.11 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.02
Forced photometry filter KEPT candidate at 05:42:37.11 +55:26:33.0: ref_mag=13.08 +/- 0.02 new_mean_mag=12.1305 delta=0.95 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 06:04:44.89 +57:46:52.6: 12.68 +/- 0.02 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 06:04:44.89 +57:46:52.6: 12.68 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.01
Forced photometry filter KEPT candidate at 06:04:44.89 +57:46:52.6: ref_mag=12.68 +/- 0.01 new_mean_mag=11.7736 delta=0.91 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:37:39.51 +54:06:44.7: 14.29 +/- 0.06 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:34:37.49 +53:38:03.0: 14.10 +/- 0.05 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:37:03.11 +53:58:27.8: 14.06 +/- 0.05 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:37:39.51 +54:06:44.7: 14.23 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.26 +/- 0.04
Forced photometry filter KEPT candidate at 05:37:39.51 +54:06:44.7: ref_mag=14.26 +/- 0.04 new_mean_mag=13.0332 delta=1.22 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:34:37.49 +53:38:03.0: 14.03 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.06 +/- 0.03
Forced photometry filter KEPT candidate at 05:34:37.49 +53:38:03.0: ref_mag=14.06 +/- 0.03 new_mean_mag=12.9874 delta=1.07 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:37:03.11 +53:58:27.8: 14.07 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.06 +/- 0.03
Forced photometry filter KEPT candidate at 05:37:03.11 +53:58:27.8: ref_mag=14.06 +/- 0.03 new_mean_mag=12.8557 delta=1.21 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:34:17.98 +52:16:29.8: 14.05 +/- 0.05 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:34:17.98 +52:16:29.8: 14.13 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.08 +/- 0.04
Forced photometry filter KEPT candidate at 05:34:17.98 +52:16:29.8: ref_mag=14.08 +/- 0.04 new_mean_mag=12.9719 delta=1.11 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:40:04.30 +54:14:54.8: 14.01 +/- 0.05 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:40:04.30 +54:14:54.8: 14.12 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.06 +/- 0.03
Forced photometry filter KEPT candidate at 05:40:04.30 +54:14:54.8: ref_mag=14.06 +/- 0.03 new_mean_mag=12.9625 delta=1.10 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:48:48.39 +56:10:18.3: 14.01 +/- 0.05 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:48:48.39 +56:10:18.3: 14.02 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.02 +/- 0.03
Forced photometry filter KEPT candidate at 05:48:48.39 +56:10:18.3: ref_mag=14.02 +/- 0.03 new_mean_mag=12.8312 delta=1.18 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:31:50.03 +50:50:01.1: 13.97 +/- 0.05 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:31:50.03 +50:50:01.1: 13.92 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.94 +/- 0.03
Forced photometry filter KEPT candidate at 05:31:50.03 +50:50:01.1: ref_mag=13.94 +/- 0.03 new_mean_mag=12.8919 delta=1.05 (need > 0.90)
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-48-02_20.00sec_-14.90C_LIGHT_0235.fits at 05:35:35.37 +50:54:50.5: 13.55 +/- 0.03 detection
Forced photometry on wcs_Aur-01-Q1b1x1_2026-01-17_23-49-01_20.00sec_-15.00C_LIGHT_0236.fits at 05:35:35.37 +50:54:50.5: 13.53 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.54 +/- 0.02
Forced photometry filter REJECTED candidate at 05:35:35.37 +50:54:50.5: ref_mag=13.54 +/- 0.02 new_mean_mag=12.7772 delta=0.76 (need > 0.90)
Adding exclusion_list_local.txt__out04720.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05588.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out100501.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out101692.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out101987.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out110197.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11377.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11688.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118421.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out119390.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out122852.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out123658.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out129037.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13365.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133727.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134674.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15005.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out18141.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out18709.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19167.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21204.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21588.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23771.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24901.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29808.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31427.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32519.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32895.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33783.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33905.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37362.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37870.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37995.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39838.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40145.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40376.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out43450.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out45914.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46773.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50770.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52538.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53915.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55080.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55543.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out58900.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out59273.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out59637.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out61761.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out62376.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out63595.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out63827.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out65077.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out65122.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67824.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out68754.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out71270.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out71599.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out72926.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out73862.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out78337.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out82158.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out85133.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out87959.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out96581.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 100s
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: 33s
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Considering the candidate 164923_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
The candidate 164923_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301 did not pass the final checks
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Considering the candidate 164924_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
The candidate 164924_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301 did not pass the final checks
**** FOUND 05:17:19.29 +51:37:36.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 164926_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
The candidate 164926_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301 did not pass the final checks
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Considering the candidate 164929_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
The candidate 164929_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301 did not pass the final checks
**** FOUND 05:46:55.72 +58:48:29.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 164930_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
The candidate 164930_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301 did not pass the final checks
**** FOUND 05:32:17.28 +50:38:18.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 164931_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
The candidate 164931_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301 did not pass the final checks
**** FOUND 05:13:51.35 +50:38:48.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 164932_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
The candidate 164932_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301 did not pass the final checks
**** FOUND 04:42:47.88 +57:22:54.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 164933_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
The candidate 164933_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301 did not pass the final checks
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Considering the candidate 164934_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
The candidate 164934_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301 did not pass the final checks
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Considering the candidate 164980_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
The candidate 164980_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301 did not pass the final checks
**** FOUND 05:36:46.41 +54:26:38.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 165012_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
The candidate 165012_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301 did not pass the final checks
**** FOUND 05:06:21.14 +58:57:53.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 165045_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
The candidate 165045_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301 did not pass the final checks
**** FOUND 05:36:44.60 +54:23:38.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 165070_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
The candidate 165070_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301 did not pass the final checks
**** FOUND 05:55:12.97 +55:41:08.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 165085_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
The candidate 165085_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301 did not pass the final checks
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Considering the candidate 165103_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
The candidate 165103_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301 did not pass the final checks
**** FOUND 04:51:44.65 +50:40:25.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 165111_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
The candidate 165111_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301 did not pass the final checks
**** FOUND 04:52:27.08 +51:22:56.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 165117_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
The candidate 165117_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301 did not pass the final checks
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Considering the candidate 165121_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
The candidate 165121_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301 did not pass the final checks
**** FOUND 05:31:45.73 +51:02:29.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 165156_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
The candidate 165156_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301 did not pass the final checks
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Considering the candidate 165182_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
The candidate 165182_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301 did not pass the final checks
**** FOUND 05:21:46.40 +53:12:12.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 165185_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
The candidate 165185_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301 did not pass the final checks
**** FOUND 05:17:04.99 +53:35:11.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 165198_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
The candidate 165198_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301 did not pass the final checks
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Considering the candidate 165219_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
The candidate 165219_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301 did not pass the final checks
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Considering the candidate 165227_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
The candidate 165227_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301 did not pass the final checks
**** FOUND 05:59:55.34 +54:33:29.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 165233_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
The candidate 165233_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301 did not pass the final checks
**** FOUND 04:48:33.75 +51:41:17.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 165234_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
The candidate 165234_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301 did not pass the final checks
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Considering the candidate 165239_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
The candidate 165239_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301 did not pass the final checks
**** FOUND 05:55:03.34 +55:42:10.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 165242_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
The candidate 165242_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301 did not pass the final checks
**** FOUND 05:46:45.98 +56:56:36.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 165247_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
The candidate 165247_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301 did not pass the final checks
**** FOUND 06:32:37.00 +57:49:49.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 165260_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
The candidate 165260_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301 did not pass the final checks
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Considering the candidate 165281_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
The candidate 165281_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301 did not pass the final checks
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Considering the candidate 165288_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
The candidate 165288_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301 did not pass the final checks
**** FOUND 04:57:20.50 +53:27:38.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 165298_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
The candidate 165298_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301 did not pass the final checks
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Considering the candidate 165300_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
The candidate 165300_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301 did not pass the final checks
**** FOUND 05:47:00.33 +56:56:35.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 165307_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
The candidate 165307_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301 did not pass the final checks
**** FOUND 05:14:53.39 +51:20:56.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 165325_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
The candidate 165325_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301 did not pass the final checks
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Considering the candidate 81125_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
The candidate 81125_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301 did not pass the final checks
**** FOUND 05:33:57.94 +52:48:27.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 29808_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
Preparing report for the candidate 29808_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
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Considering the candidate 85133_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
Preparing report for the candidate 85133_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
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Considering the candidate 23771_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
Preparing report for the candidate 23771_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
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Considering the candidate 31427_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
Preparing report for the candidate 31427_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
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Considering the candidate 100501_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
Preparing report for the candidate 100501_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
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Considering the candidate 46773_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
Preparing report for the candidate 46773_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
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Considering the candidate 134674_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
Preparing report for the candidate 134674_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
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Considering the candidate 18709_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
Preparing report for the candidate 18709_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
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Considering the candidate 37870_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
Preparing report for the candidate 37870_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
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Considering the candidate 71599_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
Preparing report for the candidate 71599_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
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Considering the candidate 71270_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
Preparing report for the candidate 71270_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
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Considering the candidate 101987_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
Preparing report for the candidate 101987_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
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Considering the candidate 19167_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
Preparing report for the candidate 19167_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
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Considering the candidate 123658_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
Preparing report for the candidate 123658_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
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Considering the candidate 33905_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
Preparing report for the candidate 33905_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
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Considering the candidate 62376_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
Preparing report for the candidate 62376_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
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Considering the candidate 55543_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
Preparing report for the candidate 55543_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
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Considering the candidate 63595_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
Preparing report for the candidate 63595_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
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Considering the candidate 78337_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
Preparing report for the candidate 78337_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
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Considering the candidate 133727_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
Preparing report for the candidate 133727_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
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Considering the candidate 82158_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
Preparing report for the candidate 82158_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
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Considering the candidate 53915_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
Preparing report for the candidate 53915_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
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Considering the candidate 58900_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
Preparing report for the candidate 58900_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
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Considering the candidate 32895_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
Preparing report for the candidate 32895_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
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Considering the candidate 119390_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
Preparing report for the candidate 119390_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
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Considering the candidate 72926_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
Preparing report for the candidate 72926_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
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Considering the candidate 115804_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
The candidate 115804_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301 did not pass the final checks
**** FOUND 05:26:08.27 +50:18:38.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 118421_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
Preparing report for the candidate 118421_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
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Considering the candidate 21204_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
Preparing report for the candidate 21204_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
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Considering the candidate 65122_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
Preparing report for the candidate 65122_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
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Considering the candidate 40376_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
Preparing report for the candidate 40376_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
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Considering the candidate 110197_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
Preparing report for the candidate 110197_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
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Considering the candidate 96581_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
Preparing report for the candidate 96581_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
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Considering the candidate 38016_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
The candidate 38016_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301 did not pass the final checks
**** FOUND 05:39:50.94 +55:53:06.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 40145_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
Preparing report for the candidate 40145_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
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Considering the candidate 50770_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
Preparing report for the candidate 50770_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
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Considering the candidate 24901_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
Preparing report for the candidate 24901_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
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Considering the candidate 37362_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
Preparing report for the candidate 37362_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
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Considering the candidate 73862_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
Preparing report for the candidate 73862_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
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Considering the candidate 65077_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
Preparing report for the candidate 65077_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
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Considering the candidate 55080_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
Preparing report for the candidate 55080_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
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Considering the candidate 29351_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
The candidate 29351_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301 did not pass the final checks
**** FOUND 05:34:27.33 +56:41:09.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 45914_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
Preparing report for the candidate 45914_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
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Considering the candidate 116143_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
The candidate 116143_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301 did not pass the final checks
**** FOUND 05:32:37.21 +50:14:48.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 37995_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
Preparing report for the candidate 37995_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
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Considering the candidate 43800_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
The candidate 43800_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301 did not pass the final checks
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Considering the candidate 13365_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
Preparing report for the candidate 13365_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
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Considering the candidate 21588_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
Preparing report for the candidate 21588_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
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Considering the candidate 52538_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
Preparing report for the candidate 52538_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
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Considering the candidate 140387_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
The candidate 140387_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301 did not pass the final checks
Rejecting candidate due to large distance (40.1") between the two second-epoch detections
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Considering the candidate 11377_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
Preparing report for the candidate 11377_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
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Considering the candidate 59273_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
Preparing report for the candidate 59273_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
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Considering the candidate 15005_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
Preparing report for the candidate 15005_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
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Considering the candidate 41496_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
The candidate 41496_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301 did not pass the final checks
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Considering the candidate 05588_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
Preparing report for the candidate 05588_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
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Considering the candidate 39838_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
Preparing report for the candidate 39838_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
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Considering the candidate 32519_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
Preparing report for the candidate 32519_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
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Considering the candidate 18141_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
Preparing report for the candidate 18141_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
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Considering the candidate 101692_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
Preparing report for the candidate 101692_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
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Considering the candidate 42859_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
The candidate 42859_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301 did not pass the final checks
**** FOUND 05:35:49.72 +55:32:43.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 140930_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
The candidate 140930_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301 did not pass the final checks
Rejecting candidate due to large distance (39.0") between the two second-epoch detections
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Considering the candidate 39295_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
The candidate 39295_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301 did not pass the final checks
**** FOUND 06:00:31.07 +55:27:13.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 129037_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
Preparing report for the candidate 129037_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
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Considering the candidate 04720_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
Preparing report for the candidate 04720_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
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Considering the candidate 129425_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
The candidate 129425_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301 did not pass the final checks
Rejecting candidate due to large distance (45.8") between the two second-epoch detections
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Considering the candidate 23347_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
The candidate 23347_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301 did not pass the final checks
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Considering the candidate 67824_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
Preparing report for the candidate 67824_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
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Considering the candidate 43450_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
Preparing report for the candidate 43450_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
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Considering the candidate 79981_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
The candidate 79981_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301 did not pass the final checks
**** FOUND 05:41:35.93 +52:48:47.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 01845_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
The candidate 01845_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301 did not pass the final checks
**** FOUND 06:07:25.01 +58:39:25.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 90823_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
The candidate 90823_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301 did not pass the final checks
**** FOUND 05:36:56.71 +52:02:31.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33733_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
The candidate 33733_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301 did not pass the final checks
**** FOUND 05:00:51.63 +56:10:52.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 11688_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
Preparing report for the candidate 11688_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
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Considering the candidate 114037_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
The candidate 114037_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301 did not pass the final checks
**** FOUND 05:27:04.42 +50:07:28.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 34009_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
The candidate 34009_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301 did not pass the final checks
Rejecting candidate due to large distance (36.5") between the two second-epoch detections
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Considering the candidate 09093_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
The candidate 09093_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301 did not pass the final checks
Rejecting candidate due to large distance (33.9") between the two second-epoch detections
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Considering the candidate 61761_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
Preparing report for the candidate 61761_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
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Considering the candidate 68754_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
Preparing report for the candidate 68754_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
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Considering the candidate 63827_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
Preparing report for the candidate 63827_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
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Considering the candidate 87959_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
Preparing report for the candidate 87959_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
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Considering the candidate 126898_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
The candidate 126898_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301 did not pass the final checks
**** FOUND 05:29:11.21 +51:10:36.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 59637_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
Preparing report for the candidate 59637_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
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Considering the candidate 33783_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
Preparing report for the candidate 33783_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
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Considering the candidate 122852_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
Preparing report for the candidate 122852_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
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Considering the candidate 112905_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
The candidate 112905_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301 did not pass the final checks
**** FOUND 04:54:15.24 +49:54:01.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 123935_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301
The candidate 123935_fd_Aur-01-Q1b1x1_2026-08-17_02-23-26_20.00sec_-0.00C_LIGHTs_0301 did not pass the final checks
make_report_in_HTML.sh Phase 2 (HTML assembly): 6s
make_report_in_HTML.sh TOTAL: 139s
Prepared the HTML report for the field Aur-01-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
06:02:41.20 +58:29:42.4
06:04:24.29 +58:22:52.0
04:54:24.73 +50:50:08.6
05:26:01.58 +51:33:53.2
04:57:45.79 +51:36:13.2
05:20:36.38 +49:48:13.2
06:03:34.05 +57:50:33.0
06:04:44.89 +57:46:52.6
04:57:46.41 +50:25:34.1
05:32:04.11 +50:32:36.9
05:31:50.03 +50:50:01.1
05:32:47.75 +50:53:24.3
05:34:17.21 +51:20:54.3
06:02:54.74 +57:40:37.8
05:26:53.09 +51:50:32.7
05:34:52.94 +51:53:03.7
05:57:39.19 +57:38:03.1
05:57:54.51 +57:21:52.1
06:01:21.71 +57:12:11.1
05:54:47.45 +57:19:44.9
05:53:27.12 +57:10:27.0
05:55:06.04 +57:07:01.8
05:53:22.42 +56:57:07.2
05:52:07.90 +56:52:53.8
05:50:19.24 +56:29:05.9
05:43:02.29 +56:26:26.1
05:42:40.50 +56:20:38.0
05:50:07.59 +56:13:10.7
05:48:48.39 +56:10:18.3
05:50:02.10 +56:08:33.1
05:38:55.51 +55:58:52.7
05:47:18.83 +55:50:29.5
05:46:54.01 +55:50:01.2
05:40:22.07 +55:45:24.0
05:46:04.02 +55:39:55.4
05:44:05.84 +55:40:28.7
05:42:37.11 +55:26:33.0
05:43:16.88 +55:14:46.9
05:44:15.90 +55:09:50.1
05:42:54.04 +54:52:53.3
05:42:46.09 +54:44:39.6
05:41:29.43 +54:38:58.8
05:41:05.59 +54:34:29.4
05:39:37.99 +54:33:15.3
05:40:15.14 +54:17:29.3
05:35:01.42 +54:18:43.4
05:40:04.30 +54:14:54.8
05:37:39.51 +54:06:44.7
05:40:14.81 +54:02:48.2
05:37:53.88 +53:58:59.9
05:37:03.11 +53:58:27.8
05:35:41.59 +53:53:29.7
05:35:32.95 +53:53:37.0
05:38:32.79 +53:39:11.5
05:34:37.49 +53:38:03.0
05:40:38.78 +53:24:10.7
05:34:58.07 +53:25:58.2
05:43:20.94 +53:14:52.8
05:35:22.99 +53:16:01.5
05:31:42.82 +52:59:28.1
05:38:46.03 +52:40:16.0
05:29:54.09 +52:31:33.7
05:34:17.98 +52:16:29.8
05:07:34.64 +49:24:22.7
########### Completed Aur-01-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 ####
05:50:19.24 +56:29:05.9
05:29:54.09 +52:31:33.7
05:53:22.42 +56:57:07.2
05:43:02.29 +56:26:26.1
04:54:24.73 +50:50:08.6
05:44:15.90 +55:09:50.1
05:34:52.94 +51:53:03.7
06:01:21.71 +57:12:11.1
05:47:18.83 +55:50:29.5
05:34:58.07 +53:25:58.2
05:40:38.78 +53:24:10.7
04:57:45.79 +51:36:13.2
05:54:47.45 +57:19:44.9
05:32:47.75 +50:53:24.3
05:50:02.10 +56:08:33.1
05:40:14.81 +54:02:48.2
05:39:37.99 +54:33:15.3
05:37:53.88 +53:58:59.9
05:31:42.82 +52:59:28.1
05:26:53.09 +51:50:32.7
05:38:46.03 +52:40:16.0
05:41:29.43 +54:38:58.8
05:40:15.14 +54:17:29.3
05:50:07.59 +56:13:10.7
05:32:04.11 +50:32:36.9
05:43:20.94 +53:14:52.8
04:57:46.41 +50:25:34.1
05:53:27.12 +57:10:27.0
05:35:32.95 +53:53:37.0
05:44:05.84 +55:40:28.7
05:20:36.38 +49:48:13.2
05:07:34.64 +49:24:22.7
05:46:04.02 +55:39:55.4
05:42:54.04 +54:52:53.3
05:52:07.90 +56:52:53.8
05:38:55.51 +55:58:52.7
05:35:22.99 +53:16:01.5
05:35:41.59 +53:53:29.7
05:41:05.59 +54:34:29.4
05:43:16.88 +55:14:46.9
05:46:54.01 +55:50:01.2
06:02:54.74 +57:40:37.8
05:55:06.04 +57:07:01.8
05:42:46.09 +54:44:39.6
06:03:34.05 +57:50:33.0
05:35:01.42 +54:18:43.4
05:57:39.19 +57:38:03.1
06:04:24.29 +58:22:52.0
05:40:22.07 +55:45:24.0
05:42:40.50 +56:20:38.0
05:57:54.51 +57:21:52.1
05:26:01.58 +51:33:53.2
05:34:17.21 +51:20:54.3
06:02:41.20 +58:29:42.4
05:38:32.79 +53:39:11.5
05:42:37.11 +55:26:33.0
06:04:44.89 +57:46:52.6
05:37:39.51 +54:06:44.7
05:34:37.49 +53:38:03.0
05:37:03.11 +53:58:27.8
05:34:17.98 +52:16:29.8
05:40:04.30 +54:14:54.8
05:48:48.39 +56:10:18.3
05:31:50.03 +50:50:01.1
###################################################################################
05:50:19.24 +56:29:05.9 -- not an asteroid (will add it to exclusion list)
05:29:54.09 +52:31:33.7 -- not an asteroid (will add it to exclusion list)
05:53:22.42 +56:57:07.2 -- not an asteroid (will add it to exclusion list)
05:43:02.29 +56:26:26.1 -- not an asteroid (will add it to exclusion list)
04:54:24.73 +50:50:08.6 -- not an asteroid (will add it to exclusion list)
05:44:15.90 +55:09:50.1 -- not an asteroid (will add it to exclusion list)
05:34:52.94 +51:53:03.7 -- not an asteroid (will add it to exclusion list)
06:01:21.71 +57:12:11.1 -- not an asteroid (will add it to exclusion list)
05:47:18.83 +55:50:29.5 -- not an asteroid (will add it to exclusion list)
05:34:58.07 +53:25:58.2 -- not an asteroid (will add it to exclusion list)
05:40:38.78 +53:24:10.7 -- not an asteroid (will add it to exclusion list)
04:57:45.79 +51:36:13.2 -- not an asteroid (will add it to exclusion list)
05:54:47.45 +57:19:44.9 -- not an asteroid (will add it to exclusion list)
05:32:47.75 +50:53:24.3 -- not an asteroid (will add it to exclusion list)
05:50:02.10 +56:08:33.1 -- not an asteroid (will add it to exclusion list)
05:40:14.81 +54:02:48.2 -- not an asteroid (will add it to exclusion list)
05:39:37.99 +54:33:15.3 -- not an asteroid (will add it to exclusion list)
05:37:53.88 +53:58:59.9 -- not an asteroid (will add it to exclusion list)
05:31:42.82 +52:59:28.1 -- not an asteroid (will add it to exclusion list)
05:26:53.09 +51:50:32.7 -- not an asteroid (will add it to exclusion list)
05:38:46.03 +52:40:16.0 -- not an asteroid (will add it to exclusion list)
05:41:29.43 +54:38:58.8 -- not an asteroid (will add it to exclusion list)
05:40:15.14 +54:17:29.3 -- not an asteroid (will add it to exclusion list)
05:50:07.59 +56:13:10.7 -- not an asteroid (will add it to exclusion list)
05:32:04.11 +50:32:36.9 -- not an asteroid (will add it to exclusion list)
05:43:20.94 +53:14:52.8 -- not an asteroid (will add it to exclusion list)
04:57:46.41 +50:25:34.1 -- not an asteroid (will add it to exclusion list)
05:53:27.12 +57:10:27.0 -- not an asteroid (will add it to exclusion list)
05:35:32.95 +53:53:37.0 -- not an asteroid (will add it to exclusion list)
05:44:05.84 +55:40:28.7 -- not an asteroid (will add it to exclusion list)
05:20:36.38 +49:48:13.2 -- not an asteroid (will add it to exclusion list)
05:07:34.64 +49:24:22.7 -- not an asteroid (will add it to exclusion list)
05:46:04.02 +55:39:55.4 -- not an asteroid (will add it to exclusion list)
05:42:54.04 +54:52:53.3 -- not an asteroid (will add it to exclusion list)
05:52:07.90 +56:52:53.8 -- not an asteroid (will add it to exclusion list)
05:38:55.51 +55:58:52.7 -- not an asteroid (will add it to exclusion list)
05:35:22.99 +53:16:01.5 -- not an asteroid (will add it to exclusion list)
05:35:41.59 +53:53:29.7 -- not an asteroid (will add it to exclusion list)
05:41:05.59 +54:34:29.4 -- not an asteroid (will add it to exclusion list)
05:43:16.88 +55:14:46.9 -- not an asteroid (will add it to exclusion list)
05:46:54.01 +55:50:01.2 -- not an asteroid (will add it to exclusion list)
06:02:54.74 +57:40:37.8 -- not an asteroid (will add it to exclusion list)
05:55:06.04 +57:07:01.8 -- not an asteroid (will add it to exclusion list)
05:42:46.09 +54:44:39.6 -- not an asteroid (will add it to exclusion list)
06:03:34.05 +57:50:33.0 -- not an asteroid (will add it to exclusion list)
05:35:01.42 +54:18:43.4 -- not an asteroid (will add it to exclusion list)
05:57:39.19 +57:38:03.1 -- not an asteroid (will add it to exclusion list)
06:04:24.29 +58:22:52.0 -- not an asteroid (will add it to exclusion list)
05:40:22.07 +55:45:24.0 -- not an asteroid (will add it to exclusion list)
05:42:40.50 +56:20:38.0 -- not an asteroid (will add it to exclusion list)
05:57:54.51 +57:21:52.1 -- not an asteroid (will add it to exclusion list)
05:26:01.58 +51:33:53.2 -- not an asteroid (will add it to exclusion list)
05:34:17.21 +51:20:54.3 -- not an asteroid (will add it to exclusion list)
06:02:41.20 +58:29:42.4 -- not an asteroid (will add it to exclusion list)
05:38:32.79 +53:39:11.5 -- not an asteroid (will add it to exclusion list)
05:42:37.11 +55:26:33.0 -- not an asteroid (will add it to exclusion list)
06:04:44.89 +57:46:52.6 -- not an asteroid (will add it to exclusion list)
05:37:39.51 +54:06:44.7 -- not an asteroid (will add it to exclusion list)
05:34:37.49 +53:38:03.0 -- not an asteroid (will add it to exclusion list)
05:37:03.11 +53:58:27.8 -- not an asteroid (will add it to exclusion list)
05:34:17.98 +52:16:29.8 -- not an asteroid (will add it to exclusion list)
05:40:04.30 +54:14:54.8 -- not an asteroid (will add it to exclusion list)
05:48:48.39 +56:10:18.3 -- not an asteroid (will add it to exclusion list)
05:31:50.03 +50:50:01.1 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
04:54:24.73 +50:50:08.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:45.79 +51:36:13.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:46.41 +50:25:34.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:07:34.64 +49:24:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:20:36.38 +49:48:13.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:26:01.58 +51:33:53.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:26:53.09 +51:50:32.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:29:54.09 +52:31:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:31:42.82 +52:59:28.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:31:50.03 +50:50:01.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:32:04.11 +50:32:36.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:32:47.75 +50:53:24.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:34:17.21 +51:20:54.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:34:17.98 +52:16:29.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:34:37.49 +53:38:03.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:34:52.94 +51:53:03.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:34:58.07 +53:25:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:35:01.42 +54:18:43.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:35:22.99 +53:16:01.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:35:32.95 +53:53:37.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:35:41.59 +53:53:29.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:03.11 +53:58:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:39.51 +54:06:44.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:53.88 +53:58:59.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:38:32.79 +53:39:11.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:38:46.03 +52:40:16.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:38:55.51 +55:58:52.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:39:37.99 +54:33:15.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:40:04.30 +54:14:54.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:40:14.81 +54:02:48.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:40:15.14 +54:17:29.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:40:22.07 +55:45:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:40:38.78 +53:24:10.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:41:05.59 +54:34:29.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:41:29.43 +54:38:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:42:37.11 +55:26:33.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:42:40.50 +56:20:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:42:46.09 +54:44:39.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:42:54.04 +54:52:53.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:43:02.29 +56:26:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:43:16.88 +55:14:46.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:43:20.94 +53:14:52.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:44:05.84 +55:40:28.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:44:15.90 +55:09:50.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:46:04.02 +55:39:55.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:46:54.01 +55:50:01.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:47:18.83 +55:50:29.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:48.39 +56:10:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:02.10 +56:08:33.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:07.59 +56:13:10.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:19.24 +56:29:05.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:07.90 +56:52:53.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:22.42 +56:57:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:27.12 +57:10:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:54:47.45 +57:19:44.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:06.04 +57:07:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:39.19 +57:38:03.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:54.51 +57:21:52.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:21.71 +57:12:11.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:02:41.20 +58:29:42.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:02:54.74 +57:40:37.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:03:34.05 +57:50:33.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:04:24.29 +58:22:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:04:44.89 +57:46:52.6 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
04:54:24.73 +50:50:08.6 -- a known variable star
04:57:45.79 +51:36:13.2 -- not a known variable star
04:57:46.41 +50:25:34.1 -- not a known variable star
05:07:34.64 +49:24:22.7 -- not a known variable star
05:20:36.38 +49:48:13.2 -- a known variable star
05:26:01.58 +51:33:53.2 -- a known variable star
05:26:53.09 +51:50:32.7 -- a known variable star
05:29:54.09 +52:31:33.7 -- not a known variable star
05:31:42.82 +52:59:28.1 -- not a known variable star
05:31:50.03 +50:50:01.1 -- not a known variable star
05:32:04.11 +50:32:36.9 -- a known variable star
05:32:47.75 +50:53:24.3 -- not a known variable star
05:34:17.21 +51:20:54.3 -- a known variable star
05:34:17.98 +52:16:29.8 -- not a known variable star
05:34:37.49 +53:38:03.0 -- not a known variable star
05:34:52.94 +51:53:03.7 -- not a known variable star
05:34:58.07 +53:25:58.2 -- not a known variable star
05:35:01.42 +54:18:43.4 -- not a known variable star
05:35:22.99 +53:16:01.5 -- a known variable star
05:35:32.95 +53:53:37.0 -- not a known variable star
05:35:41.59 +53:53:29.7 -- not a known variable star
05:37:03.11 +53:58:27.8 -- not a known variable star
05:37:39.51 +54:06:44.7 -- not a known variable star
05:37:53.88 +53:58:59.9 -- not a known variable star
05:38:32.79 +53:39:11.5 -- a known variable star
05:38:46.03 +52:40:16.0 -- a known variable star
05:38:55.51 +55:58:52.7 -- not a known variable star
05:39:37.99 +54:33:15.3 -- not a known variable star
05:40:04.30 +54:14:54.8 -- not a known variable star
05:40:14.81 +54:02:48.2 -- not a known variable star
05:40:15.14 +54:17:29.3 -- not a known variable star
05:40:22.07 +55:45:24.0 -- not a known variable star
05:40:38.78 +53:24:10.7 -- not a known variable star
05:41:05.59 +54:34:29.4 -- not a known variable star
05:41:29.43 +54:38:58.8 -- not a known variable star
05:42:37.11 +55:26:33.0 -- a known variable star
05:42:40.50 +56:20:38.0 -- not a known variable star
05:42:46.09 +54:44:39.6 -- not a known variable star
05:42:54.04 +54:52:53.3 -- not a known variable star
05:43:02.29 +56:26:26.1 -- not a known variable star
05:43:16.88 +55:14:46.9 -- not a known variable star
05:43:20.94 +53:14:52.8 -- not a known variable star
05:44:05.84 +55:40:28.7 -- not a known variable star
05:44:15.90 +55:09:50.1 -- not a known variable star
05:46:04.02 +55:39:55.4 -- not a known variable star
05:46:54.01 +55:50:01.2 -- not a known variable star
05:47:18.83 +55:50:29.5 -- not a known variable star
05:48:48.39 +56:10:18.3 -- not a known variable star
05:50:02.10 +56:08:33.1 -- not a known variable star
05:50:07.59 +56:13:10.7 -- not a known variable star
05:50:19.24 +56:29:05.9 -- not a known variable star
05:52:07.90 +56:52:53.8 -- not a known variable star
05:53:22.42 +56:57:07.2 -- not a known variable star
05:53:27.12 +57:10:27.0 -- not a known variable star
05:54:47.45 +57:19:44.9 -- not a known variable star
05:55:06.04 +57:07:01.8 -- not a known variable star
05:57:39.19 +57:38:03.1 -- not a known variable star
05:57:54.51 +57:21:52.1 -- not a known variable star
06:01:21.71 +57:12:11.1 -- not a known variable star
06:02:41.20 +58:29:42.4 -- not a known variable star
06:02:54.74 +57:40:37.8 -- not a known variable star
06:03:34.05 +57:50:33.0 -- not a known variable star
06:04:24.29 +58:22:52.0 -- not a known variable star
06:04:44.89 +57:46:52.6 -- a known variable star
Found 53 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
64 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 64 (excluding asteroids and hot pixels, 53 new), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461269.80728188 -observatory V36
09:04:40.25 +18:03:26.6 Mercury (-1.4mag)
12:33:50.62 -05:25:22.7 Venus (-4.4mag)
06:15:30.25 +23:42:22.6 Mars (1.3mag)
08:51:03.62 +18:10:28.8 Jupiter (-1.8mag)
00:55:31.57 +03:07:16.2 Saturn (0.5mag)
04:12:38.85 +20:59:19.1 Uranus (5.7mag)
00:15:30.73 +00:08:55.9 Neptune (7.7mag)
20:27:17.52 -23:33:30.8 Pluto (14.5mag)
13:12:40.73 -12:50:13.1 Moon (-9.5mag)
-rw-r--r-- 1 apache apache 362 Aug 17 02:28 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461269.80728188:
08:51:01.74 +18:10:37.4 Io (6.1mag)
08:50:55.67 +18:11:05.7 Europa (6.3mag)
08:51:05.77 +18:10:17.2 Ganymede (5.6mag)
08:50:54.46 +18:11:07.9 Callisto (6.8mag)
08:48:31.66 +18:15:25.7 Himalia (15.7mag)
08:51:07.46 +18:10:12.3 Thebe (16.6mag)
08:48:08.94 +18:12:12.0 Elara (17.7mag)
08:55:12.33 +17:45:50.8 Pasiphae (17.9mag)
08:53:37.71 +18:22:49.7 Carme (19.0mag)
00:55:43.59 +03:06:58.4 Titan (8.4mag)
00:55:35.30 +03:06:59.5 Rhea (9.7mag)
00:56:01.84 +03:07:57.7 Iapetus (11.1mag)
00:55:46.29 +03:06:47.4 Hyperion (14.4mag)
00:54:42.51 +02:59:17.8 Phoebe (16.4mag)
-rw-r--r-- 1 apache apache 568 Aug 17 02:28 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461269.80728188:
19:43:53.92 -17:44:44.7 JWST
17:58:20.17 +30:13:49.0 Chandra
05:19:01.62 +43:20:56.0 XMM-Newton
-rw-r--r-- 1 apache apache 96 Aug 17 02:28 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461269.80728188 -observatory V36
03:23:24.82 +18:05:26.0 17.6mag P/1996 R2 (Lagerkvist)
18:00:04.74 -34:32:36.0 14.1mag P/2010 H2 (Vales)
07:02:04.51 -69:15:51.7 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:12:03.69 +33:11:29.7 17.7mag C/2017 K2 (PANSTARRS)
04:08:50.11 +41:00:55.8 17.2mag P/2021 N1 (ZTF)
22:31:01.41 +30:48:43.5 17.3mag C/2022 E2 (ATLAS)
06:52:16.83 +26:22:42.2 16.8mag C/2022 N2 (PANSTARRS)
10:30:00.30 +28:04:03.4 17.0mag C/2022 QE78 (ATLAS)
09:34:56.73 +05:18:30.7 18.0mag C/2022 R6 (PANSTARRS)
15:14:19.41 -12:39:24.4 17.9mag P/2023 B1 (PANSTARRS)
20:59:13.15 +64:51:10.5 17.9mag C/2023 H5 (Lemmon)
15:39:54.21 -13:46:31.4 14.5mag C/2023 R1 (PANSTARRS)
08:18:01.25 +31:45:57.6 15.5mag C/2024 E1 (Wierzchos)
15:05:54.79 +15:33:08.3 17.8mag C/2024 G6 (ATLAS)
18:52:15.34 +43:26:06.3 13.7mag C/2024 J3 (ATLAS)
20:57:04.73 +49:36:33.1 17.5mag C/2024 R4 (PANSTARRS)
05:22:09.01 -12:54:05.3 15.4mag C/2024 T5 (ATLAS)
07:01:49.67 +22:32:01.7 17.9mag C/2025 J1 (Borisov)
10:45:49.17 +20:18:34.1 17.2mag C/2025 V2 (Rankin)
13:03:54.03 +01:43:23.8 16.9mag C/2025 Y1 (ATLAS)
16:05:29.70 +76:53:16.0 16.6mag C/2026 A2 (Bok)
03:09:42.78 +46:19:21.7 17.2mag C/2026 B2 (Sun-Gao)
11:54:26.97 +09:27:44.5 17.4mag A/2026 E1
22:07:42.84 -30:45:32.5 7.0mag 10P/Tempel
11:34:31.40 -03:58:46.5 16.3mag 29P/Schwassmann-Wachmann
11:26:10.62 +01:40:08.9 17.4mag 63P/Wild
00:52:58.26 -05:50:22.4 15.4mag 65P/Gunn
05:55:50.97 +20:27:21.1 13.7mag 78P/Gehrels
20:29:54.74 -24:31:01.9 17.6mag 84P/Giclas
03:08:38.66 +14:17:01.3 16.8mag 88P/Howell
08:18:31.26 +26:21:46.2 16.3mag 93P/Lovas
04:32:27.10 +20:25:25.6 17.3mag 112P/Urata-Niijima
06:26:18.04 +29:08:24.9 16.1mag 114P/Wiseman-Skiff
09:39:54.49 +25:02:41.6 14.9mag 123P/West-Hartley
12:02:05.11 -13:43:22.1 17.2mag 124P/Mrkos
05:49:42.96 +21:06:23.2 16.0mag 128P/Shoemaker-Holt
06:43:46.77 +18:24:49.3 17.9mag 131P/Mueller
00:01:18.76 +03:15:04.3 17.5mag 139P/Vaisala-Oterma
03:14:59.91 -18:49:10.7 13.2mag 161P/Hartley-IRAS
07:47:02.77 +38:06:17.9 16.0mag 162P/Siding Spring
12:13:28.18 +36:57:06.4 12.0mag 169P/NEAT
02:58:35.36 +09:30:58.9 17.6mag 220P/McNaught
16:47:03.32 -10:45:45.0 17.9mag 235P/LINEAR
20:17:37.37 -52:21:35.7 17.9mag 259P/Garradd
03:48:37.78 +28:53:15.1 15.3mag 260P/McNaught
07:32:32.18 +37:23:07.5 17.3mag 295P/LINEAR
15:13:52.58 +02:07:33.1 17.8mag 391P/Kowalski
09:09:09.46 +17:55:27.3 17.9mag 450P/LONEOS
-rw-r--r-- 1 apache apache 2.3K Aug 17 02:28 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
00:56:54.35 -35:55:29.40 AT2026wdy 2026-08-5.05 16.08
22:08:07.63 -53:03:58.90 AT2026wek 2026-08-3.82 17.17
14:51:51.34 +66:13:24.60 ASASSN-26ev 2026-08-2.15 14.02
12:06:50.79 -36:16:06.20 SN2026wgm 2026-08-1.73 15.61
16:56:36.90 -59:29:26.00 ASASSN-26er 2026-07-25.82 15.09
01:21:27.83 -10:37:05.00 SN2026vbh 2026-07-25.61 15.97
21:17:31.59 +22:25:50.90 ASASSN-26eq 2026-07-24.37 15.13
18:53:36.89 +16:56:43.60 ASASSN-26ep 2026-07-23.47 -4.06
12:18:47.98 -30:48:47.50 ASASSN-26et 2026-07-22.76 13.98
13:00:47.82 +15:42:17.60 SN2026uwk 2026-07-21.75 16.38
18:52:31.11 -32:28:00.90 ASASSN-26en 2026-07-21.77 14.63
14:42:58.01 -62:32:59.10 ASASSN-26es 2026-07-20.79 15.36
20:12:45.57 -32:53:13.00 ASASSN-26em 2026-07-20.94 16.83
18:54:24.33 -46:11:51.70 ASASSN-26eu 2026-07-20.93 14.86
03:18:56.99 -80:55:10.40 AT2026ugi 2026-07-20.03 17.12
18:43:58.40 +24:22:41.80 ASASSN-26eo 2026-07-19.36 16.16
04:50:01.03 -02:22:33.80 ASASSN-26ej 2026-07-16.17 17.02
18:34:55.28 -31:41:00.90 ASASSN-26ek 2026-07-16.24 15.73
17:07:43.61 -44:21:53.50 ASASSN-26el 2026-07-15.86 16.01
14:45:08.35 +24:13:12.30 ASASSN-26ei 2026-07-16.17 16.46
10:00:46.44 -32:36:31.10 AT 2023mhb 2026-07-14.73 16.67
14:39:37.45 -11:22:36.20 AT 2026unl 2026-07-15.27 17.11
10:49:42.57 -11:25:55.80 ASASSN-26eh 2026-07-14.72 16.58
19:33:53.06 -07:15:00.80 ASASSN-22le 2026-07-14.15 15.5
02:45:40.52 -27:55:30.30 ASASSN-26ef 2026-07-12.35 15.86
23:26:43.80 +04:42:39.70 SN 2026qtn 2026-07-12.22 16.47
02:19:17.26 +28:57:15.40 ASASSN-26ec 2026-07-11.53 2.78
18:31:15.56 -05:34:31.50 AT2026stb 2026-07-11.28 -1.29
13:36:08.24 +23:29:05.00 AT2026pjf 2026-07-10.18 -0.72
17:33:39.82 +04:22:36.70 SN2026pir 2026-07-9.86 -0.66
11:21:41.26 -50:33:36.30 ASASSN-26ed 2026-07-8.8 -1.3
23:41:42.11 +26:29:49.10 AT2026qil 2026-07-9.3 16.15
20:21:30.50 -32:03:40.10 ASASSN-26ee 2026-07-7.22 15.53
19:37:44.09 -05:35:42.80 AT2026ryu 2026-07-7.17 14.88
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
02:02:26.67 +32:04:22.70 AT2026ovz 2026-06-14.6 15.52
21:26:28.11 -72:31:19.50 AT2026nwc 2026-06-11 17.05
17:54:57.33 +26:32:34.20 SN 2026odc 2026-06-11.23 17.62
13:55:59.94 +17:30:37.20 SN 2026nyq 2026-06-11.1 16.24
00:50:45.14 -71:38:36.90 ASASSN-26dt 2026-06-11.13 10.22
14:42:19.73 +19:11:35.60 SN2026nyp 2026-06-10.3 16.32
12:23:23.92 +12:56:43.50 SN2026mta 2026-06-8.29 16.69
12:30:18.51 +47:12:33.20 SN2026oao 2026-06-9.32 17.02
10:51:05.21 -42:28:56.60 AT2026nvf 2026-06-8.12 16.75
13:50:22.48 -07:35:00.00 SN2026npn 2026-06-8.02 17.58
00:56:07.17 +43:01:43.20 ASASSN-26dq 2026-06-7.43 13.58
01:07:49.46 +41:59:43.70 SN 2026obc 2026-06-7.43 15.15
21:11:25.22 +14:14:31.90 ASASSN-26dr 2026-06-7.24 16.24
06:21:27.06 -65:16:42.00 ASASSN-26ds 2026-06-2.97 15.02
20:07:38.15 -21:07:05.40 SN2026mho 2026-05-25.18 -1.12
11:29:42.55 +79:01:03.10 AT2026min 2026-05-24.21 16.63
11:44:33.11 -68:48:32.90 ASASSN-26no 2026-05-24.03 8.35
19:00:42.82 -48:31:01.60 ASASSN-26dp 2026-05-22.31 -3.28
14:23:56.59 -58:37:47.40 ASASSN-26dn 2026-05-20.01 14.59
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 +22:02:03.40 AT2026lxf 2026-05-8.07 13.88
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
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
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
21:17:31.48 +22:25:51.0 TCP J21173148+2225510 2026-07-23.5577 14.8mag
00:41:24.04 +40:49:02.8 PNV J00412404+4049028 2026-07-25.0157 18.7mag
00:43:04.26 +41:02:28.6 PNV J00430426+4102286 2026-07-26.1512 20mag
14:51:51.40 +66:13:24.0 TCP J14515140+6613240 2026-07-29.2561 13.5mag
00:43:06.15 +41:22:08.2 PNV J00430615+4122082 2026-07-30.0085 19.4mag
00:41:33.23 +41:10:12.2 PNV J00413323+4110122 2026-08-02.8913 17.1mag
05:21:07.63 +23:38:19.4 TCP J05210763+2338194 2026-08-06.4109 11.2mag
22:57:17.96 +47:07:41.8 TCP J22571796+4707418 2026-08-09.3289 14.3mag
09:13:38.17 +76:28:18.1 PSN J09133817+7628181 2026-08-09.8037 15.4mag
00:43:17.29 +41:26:48.6 PNV J00431729+4126486 2026-08-14.0920 16.8mag
-rw-r--r-- 1 apache apache 190K Aug 17 02:28 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
17:33:41.626 +03:55:57.27 AT 2026wvz 2026-07-19.23 21.0254
17:50:01.721 +10:25:24.49 AT 2026wvy 2026-07-26.20 20.1407
16:10:31.606 +03:57:43.31 AT 2026wvx 2026-07-17.26 20.7944
20:33:52.488 +03:24:38.01 AT 2026wvw 2026-07-23.32 20.8661
00:41:33.169 +41:10:12.40 AT 2026wvv 2026-08-02.89 17.1
23:45:36.740 -03:05:35.56 AT 2026wvu 2026-07-25.60 21.95
22:40:08.792 -06:25:00.39 AT 2026wvt 2026-07-24.51 21.53
18:01:34.940 +35:37:53.90 AT 2026wvs 2026-07-23.31 21.74
23:25:28.465 -20:01:24.81 AT 2026wvr 2026-07-26.54 20.7
23:40:24.824 -24:40:33.31 AT 2026wvq 2026-07-26.54 20.89
21:22:15.890 -02:33:52.37 AT 2026wvp 2026-07-25.44 21.07
22:10:23.762 +16:20:18.77 AT 2026wvo 2026-07-25.45 21.13
23:06:39.906 +05:33:08.21 AT 2026wvn 2026-07-24.57 21.75
00:44:57.801 +25:20:50.30 AT 2026wvm 2026-07-23.55 21.26
23:50:27.739 -03:51:06.21 AT 2026wvl 2026-07-25.58 20.96
00:25:21.084 +26:42:45.70 AT 2026wvk 2026-07-23.55 20.96
23:37:13.087 -06:14:48.44 AT 2026wvj 2026-07-25.59 22.23
00:43:40.407 -30:43:14.55 AT 2026wvi 2026-07-26.58 20.68
22:42:59.067 -07:40:12.15 AT 2026wvh 2026-07-24.50 21.36
22:23:10.327 -02:22:08.97 AT 2026wvg 2026-07-24.49 20.89
-rw-r--r-- 1 apache apache 87K Aug 17 02:28 tns_transients_list.txt
